DOE PAGES title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Nonuniversal star formation efficiency in turbulent ISM

Abstract

Here, we present a study of a star formation prescription in which star formation efficiency depends on local gas density and turbulent velocity dispersion, as suggested by direct simulations of SF in turbulent giant molecular clouds (GMCs). We test the model using a simulation of an isolated Milky Way-sized galaxy with a self-consistent treatment of turbulence on unresolved scales. We show that this prescription predicts a wide variation of local star formation efficiency per free-fall time, $$\epsilon_{\rm ff} \sim 0.1 - 10\%$$, and gas depletion time, $$t_{\rm dep} \sim 0.1 - 10$$ Gyr. In addition, it predicts an effective density threshold for star formation due to suppression of $$\epsilon_{\rm ff}$$ in warm diffuse gas stabilized by thermal pressure. We show that the model predicts star formation rates in agreement with observations from the scales of individual star-forming regions to the kiloparsec scales. This agreement is non-trivial, as the model was not tuned in any way and the predicted star formation rates on all scales are determined by the distribution of the GMC-scale densities and turbulent velocities $$\sigma$$ in the cold gas within the galaxy, which is shaped by galactic dynamics. The broad agreement of the star formation prescription calibrated in the GMC-scale simulations with observations, both gives credence to such simulations and promises to put star formation modeling in galaxy formation simulations on a much firmer theoretical footing.

Authors:
ORCiD logo [1]; ORCiD logo [1];  [2]
  1. The Univ. of Chicago, Chicago, IL (United States)
  2. The Univ. of Chicago, Chicago, IL (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Publication Date:
Research Org.:
Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP)
OSTI Identifier:
1333137
Report Number(s):
arXiv:1512.03101; FERMILAB-PUB-16-503-A
Journal ID: ISSN 1538-4357; 1495139
Grant/Contract Number:  
AC02-07CH11359
Resource Type:
Accepted Manuscript
Journal Name:
The Astrophysical Journal (Online)
Additional Journal Information:
Journal Name: The Astrophysical Journal (Online); Journal Volume: 826; Journal Issue: 2; Journal ID: ISSN 1538-4357
Publisher:
Institute of Physics (IOP)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; galaxies: ISM; numerical; stars: formation; turbulence

Citation Formats

Semenov, Vadim A., Kravtsov, Andrey V., and Gnedin, Nickolay Y. Nonuniversal star formation efficiency in turbulent ISM. United States: N. p., 2016. Web. doi:10.3847/0004-637X/826/2/200.
Semenov, Vadim A., Kravtsov, Andrey V., & Gnedin, Nickolay Y. Nonuniversal star formation efficiency in turbulent ISM. United States. https://doi.org/10.3847/0004-637X/826/2/200
Semenov, Vadim A., Kravtsov, Andrey V., and Gnedin, Nickolay Y. Fri . "Nonuniversal star formation efficiency in turbulent ISM". United States. https://doi.org/10.3847/0004-637X/826/2/200. https://www.osti.gov/servlets/purl/1333137.
@article{osti_1333137,
title = {Nonuniversal star formation efficiency in turbulent ISM},
author = {Semenov, Vadim A. and Kravtsov, Andrey V. and Gnedin, Nickolay Y.},
abstractNote = {Here, we present a study of a star formation prescription in which star formation efficiency depends on local gas density and turbulent velocity dispersion, as suggested by direct simulations of SF in turbulent giant molecular clouds (GMCs). We test the model using a simulation of an isolated Milky Way-sized galaxy with a self-consistent treatment of turbulence on unresolved scales. We show that this prescription predicts a wide variation of local star formation efficiency per free-fall time, $\epsilon_{\rm ff} \sim 0.1 - 10\%$, and gas depletion time, $t_{\rm dep} \sim 0.1 - 10$ Gyr. In addition, it predicts an effective density threshold for star formation due to suppression of $\epsilon_{\rm ff}$ in warm diffuse gas stabilized by thermal pressure. We show that the model predicts star formation rates in agreement with observations from the scales of individual star-forming regions to the kiloparsec scales. This agreement is non-trivial, as the model was not tuned in any way and the predicted star formation rates on all scales are determined by the distribution of the GMC-scale densities and turbulent velocities $\sigma$ in the cold gas within the galaxy, which is shaped by galactic dynamics. The broad agreement of the star formation prescription calibrated in the GMC-scale simulations with observations, both gives credence to such simulations and promises to put star formation modeling in galaxy formation simulations on a much firmer theoretical footing.},
doi = {10.3847/0004-637X/826/2/200},
journal = {The Astrophysical Journal (Online)},
number = 2,
volume = 826,
place = {United States},
year = {Fri Jul 29 00:00:00 EDT 2016},
month = {Fri Jul 29 00:00:00 EDT 2016}
}

Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record

Citation Metrics:
Cited by: 87 works
Citation information provided by
Web of Science

Save / Share:

Works referenced in this record:

On the Interplay Between star Formation and Feedback in Galaxy Formation Simulations
journal, April 2015


Toward a Complete Accounting of Energy and Momentum from Stellar Feedback in Galaxy Formation Simulations
journal, May 2013

  • Agertz, Oscar; Kravtsov, Andrey V.; Leitner, Samuel N.
  • The Astrophysical Journal, Vol. 770, Issue 1
  • DOI: 10.1088/0004-637X/770/1/25

Large-scale galactic turbulence: can self-gravity drive the observed H i velocity dispersions?
journal, January 2009


Disc formation and the origin of clumpy galaxies at high redshift
journal, July 2009

  • Agertz, Oscar; Teyssier, Romain; Moore, Ben
  • Monthly Notices of the Royal Astronomical Society: Letters, Vol. 397, Issue 1
  • DOI: 10.1111/j.1745-3933.2009.00685.x

Pressure-confined clumps in magnetized molecular clouds
journal, August 1992

  • Bertoldi, Frank; McKee, Christopher F.
  • The Astrophysical Journal, Vol. 395
  • DOI: 10.1086/171638

The star Formation law in Nearby Galaxies on Sub-Kpc Scales
journal, November 2008


The State of the gas and the Relation Between gas and star Formation at low Metallicity: the Small Magellanic Cloud
journal, October 2011

  • Bolatto, Alberto D.; Leroy, Adam K.; Jameson, Katherine
  • The Astrophysical Journal, Vol. 741, Issue 1
  • DOI: 10.1088/0004-637X/741/1/12

The Resolved Properties of Extragalactic Giant Molecular Clouds
journal, October 2008

  • Bolatto, Alberto D.; Leroy, Adam K.; Rosolowsky, Erik
  • The Astrophysical Journal, Vol. 686, Issue 2
  • DOI: 10.1086/591513

ISM properties in hydrodynamic galaxy simulations: turbulence cascades, cloud formation, role of gravity and feedback: ISM properties in galaxy simulations
journal, September 2010

  • Bournaud, Frédéric; Elmegreen, Bruce G.; Teyssier, Romain
  • Monthly Notices of the Royal Astronomical Society, Vol. 409, Issue 3
  • DOI: 10.1111/j.1365-2966.2010.17370.x

A semi-analytic model of the turbulent multi-phase interstellar medium: A model of the turbulent multi-phase ISM
journal, March 2012


The small and the beautiful: how the star formation law affects galactic disc structure
journal, October 2015

  • Braun, H.; Schmidt, W.
  • Monthly Notices of the Royal Astronomical Society, Vol. 454, Issue 2
  • DOI: 10.1093/mnras/stv1856

Large-eddy simulations of isolated disc galaxies with thermal and turbulent feedback
journal, July 2014

  • Braun, H.; Schmidt, W.; Niemeyer, J. C.
  • Monthly Notices of the Royal Astronomical Society, Vol. 442, Issue 4
  • DOI: 10.1093/mnras/stu1119

A piecewise parabolic method for cosmological hydrodynamics
journal, August 1995


Galaxy formation and physical bias
journal, November 1992

  • Cen, Renyue; Ostriker, Jeremiah P.
  • The Astrophysical Journal, Vol. 399
  • DOI: 10.1086/186620

The role of Stellar Feedback in the Formation of Galaxies
journal, March 2009


The gravitational instability of an infinite homogeneous turbulent medium
journal, December 1951

  • Chandrasekhar, S.
  • Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, Vol. 210, Issue 1100, p. 26-29
  • DOI: 10.1098/rspa.1951.0228

Star formation in unbound giant molecular clouds: the origin of OB associations?
journal, May 2005


Efficient solution algorithms for the Riemann problem for real gases
journal, June 1985


Self-Perpetuating Spiral arms in disk Galaxies
journal, March 2013

  • D’Onghia, Elena; Vogelsberger, Mark; Hernquist, Lars
  • The Astrophysical Journal, Vol. 766, Issue 1
  • DOI: 10.1088/0004-637X/766/1/34

Formation of Massive Galaxies at high Redshift: cold Streams, Clumpy Disks, and Compact Spheroids
journal, September 2009


Why are most molecular clouds not gravitationally bound?: Unbound molecular clouds
journal, April 2011


Star Formation Relations in Nearby Molecular Clouds
journal, February 2014

  • Evans, Neal J.; Heiderman, Amanda; Vutisalchavakul, Nalin
  • The Astrophysical Journal, Vol. 782, Issue 2
  • DOI: 10.1088/0004-637X/782/2/114

Inefficient star formation through turbulence, magnetic fields and feedback
journal, May 2015

  • Federrath, Christoph
  • Monthly Notices of the Royal Astronomical Society, Vol. 450, Issue 4
  • DOI: 10.1093/mnras/stv941

The star Formation rate of Turbulent Magnetized Clouds: Comparing Theory, Simulations, and Observations
journal, December 2012


Modeling jet and Outflow Feedback During star Cluster Formation
journal, July 2014


Can Nonlinear Hydromagnetic Waves Support a Self-gravitating Cloud?
journal, August 1996

  • Gammie, Charles F.; Ostriker, Eve C.
  • The Astrophysical Journal, Vol. 466
  • DOI: 10.1086/177556

The velocity dispersion of giant molecular clouds. II - Mathematical and numerical refinements
journal, September 1991

  • Gammie, Charles F.; Ostriker, Jeremiah P.; Jog, Chanda J.
  • The Astrophysical Journal, Vol. 378
  • DOI: 10.1086/170458

SHORT-LIVED STAR-FORMING GIANT CLUMPS IN COSMOLOGICAL SIMULATIONS OF z ≈ 2 DISKS
journal, December 2011


Modeling Molecular Hydrogen and star Formation in Cosmological Simulations
journal, April 2009

  • Gnedin, Nickolay Y.; Tassis, Konstantinos; Kravtsov, Andrey V.
  • The Astrophysical Journal, Vol. 697, Issue 1
  • DOI: 10.1088/0004-637X/697/1/55

Bulgeless dwarf galaxies and dark matter cores from supernova-driven outflows
journal, January 2010


The star Formation rate and gas Surface Density Relation in the Milky way: Implications for Extragalactic Studies
journal, October 2010


Analytical Theory for the Initial mass Function. iii. time Dependence and star Formation rate
journal, June 2013


An analytical model for spherical galaxies and bulges
journal, June 1990

  • Hernquist, Lars
  • The Astrophysical Journal, Vol. 356
  • DOI: 10.1086/168845

Galaxies on FIRE (Feedback In Realistic Environments): stellar feedback explains cosmologically inefficient star formation
journal, September 2014

  • Hopkins, Philip F.; Kereš, Dušan; Oñorbe, José
  • Monthly Notices of the Royal Astronomical Society, Vol. 445, Issue 1
  • DOI: 10.1093/mnras/stu1738

The meaning and consequences of star formation criteria in galaxy models with resolved stellar feedback
journal, May 2013

  • Hopkins, Philip F.; Narayanan, Desika; Murray, Norman
  • Monthly Notices of the Royal Astronomical Society, Vol. 432, Issue 4
  • DOI: 10.1093/mnras/stt723

Self-regulated star formation in galaxies via momentum input from massive stars: Self-regulated star formation in galaxies
journal, September 2011

  • Hopkins, Philip F.; Quataert, Eliot; Murray, Norman
  • Monthly Notices of the Royal Astronomical Society, Vol. 417, Issue 2
  • DOI: 10.1111/j.1365-2966.2011.19306.x

Turbulence production and turbulent pressure support in the intergalactic medium: Turbulence production and pressure in the IGM
journal, April 2011


Global properties of the H  I distribution in the outer Milky Way : Planar and extra-planar gas
journal, May 2008


Dissipational galaxy formation. II - Effects of star formation
journal, June 1992


Star Formation in the Milky Way and Nearby Galaxies
journal, September 2012


The Global Schmidt Law in Star‐forming Galaxies
journal, May 1998

  • Kennicutt, Jr., Robert C.
  • The Astrophysical Journal, Vol. 498, Issue 2
  • DOI: 10.1086/305588

Fully Threaded Tree Algorithms for Adaptive Refinement Fluid Dynamics Simulations
journal, July 1998


Long-Term Evolution of Decaying Magnetohydrodynamic Turbulence in the Multiphase Interstellar Medium
journal, November 2013


The Agora High-Resolution Galaxy Simulations Comparison Project
journal, December 2013

  • Kim, Ji-hoon; Abel, Tom; Agertz, Oscar
  • The Astrophysical Journal Supplement Series, Vol. 210, Issue 1
  • DOI: 10.1088/0067-0049/210/1/14

Constrained Simulations of the Real Universe. II. Observational Signatures of Intergalactic Gas in the Local Supercluster Region
journal, June 2002

  • Kravtsov, Andrey V.; Klypin, Anatoly; Hoffman, Yehuda
  • The Astrophysical Journal, Vol. 571, Issue 2
  • DOI: 10.1086/340046

Adaptive Refinement Tree: A New High‐Resolution N ‐Body Code for Cosmological Simulations
journal, July 1997

  • Kravtsov, Andrey V.; Klypin, Anatoly A.; Khokhlov, Alexei M.
  • The Astrophysical Journal Supplement Series, Vol. 111, Issue 1
  • DOI: 10.1086/313015

A supersonic turbulence origin of Larson's laws
journal, October 2013

  • Kritsuk, A. G.; Lee, C. T.; Norman, M. L.
  • Monthly Notices of the Royal Astronomical Society, Vol. 436, Issue 4
  • DOI: 10.1093/mnras/stt1805

Comparing Numerical Methods for Isothermal Magnetized Supersonic Turbulence
journal, July 2011


A Universal, Local star Formation law in Galactic Clouds, Nearby Galaxies, High-Redshift Disks, and Starbursts
journal, December 2011

  • Krumholz, Mark R.; Dekel, Avishai; McKee, Christopher F.
  • The Astrophysical Journal, Vol. 745, Issue 1
  • DOI: 10.1088/0004-637X/745/1/69

Radiation-Hydrodynamic Simulations of the Formation of Orion-Like star Clusters. ii. the Initial mass Function from Winds, Turbulence, and Radiation
journal, July 2012

  • Krumholz, Mark R.; Klein, Richard I.; McKee, Christopher F.
  • The Astrophysical Journal, Vol. 754, Issue 1
  • DOI: 10.1088/0004-637X/754/1/71

A General Theory of Turbulence‐regulated Star Formation, from Spirals to Ultraluminous Infrared Galaxies
journal, September 2005

  • Krumholz, Mark R.; McKee, Christopher F.
  • The Astrophysical Journal, Vol. 630, Issue 1
  • DOI: 10.1086/431734

On the star Formation Rates in Molecular Clouds
journal, November 2010


Turbulence and star formation in molecular clouds
journal, April 1981


The characteristic black hole mass resulting from direct collapse in the early Universe
journal, October 2013

  • Latif, M. A.; Schleicher, D. R. G.; Schmidt, W.
  • Monthly Notices of the Royal Astronomical Society, Vol. 436, Issue 4
  • DOI: 10.1093/mnras/stt1786

Shear-improved Smagorinsky model for large-eddy simulation of wall-bounded turbulent flows
journal, January 2007


THE PANCHROMATIC HUBBLE ANDROMEDA TREASURY. XI. THE SPATIALLY RESOLVED RECENT STAR FORMATION HISTORY OF M31
journal, June 2015

  • Lewis, Alexia R.; Dolphin, Andrew E.; Dalcanton, Julianne J.
  • The Astrophysical Journal, Vol. 805, Issue 2
  • DOI: 10.1088/0004-637X/805/2/183

Kinetic Energy Decay Rates of Supersonic and Super-Alfvénic Turbulence in Star-Forming Clouds
journal, March 1998

  • Mac Low, Mordecai-Mark; Klessen, Ralf S.; Burkert, Andreas
  • Physical Review Letters, Vol. 80, Issue 13
  • DOI: 10.1103/PhysRevLett.80.2754

Simulations of Pregalactic Structure Formation with Radiative Feedback
journal, February 2001

  • Machacek, Marie E.; Bryan, Greg L.; Abel, Tom
  • The Astrophysical Journal, Vol. 548, Issue 2
  • DOI: 10.1086/319014

Adaptively Refined Large eddy Simulations of a Galaxy Cluster: Turbulence Modeling and the Physics of the Intracluster Medium
journal, November 2009


Supernova feedback in an inhomogeneous interstellar medium
journal, April 2015

  • Martizzi, Davide; Faucher-Giguère, Claude-André; Quataert, Eliot
  • Monthly Notices of the Royal Astronomical Society, Vol. 450, Issue 1
  • DOI: 10.1093/mnras/stv562

Gas Kinematics on Giant Molecular Cloud Scales in m51 with Paws: Cloud Stabilization Through Dynamical Pressure
journal, November 2013

  • Meidt, Sharon E.; Schinnerer, Eva; García-Burillo, Santiago
  • The Astrophysical Journal, Vol. 779, Issue 1
  • DOI: 10.1088/0004-637X/779/1/45

The initial mass function and stellar birthrate in the solar neighborhood
journal, September 1979

  • Miller, G. E.; Scalo, J. M.
  • The Astrophysical Journal Supplement Series, Vol. 41
  • DOI: 10.1086/190629

The distribution of the ISM in the Milky Way: A three-dimensional large-scale model
journal, September 2006


Star Formation Efficiencies and Lifetimes of Giant Molecular Clouds in the Milky way
journal, February 2011


Three-dimensional distribution of the ISM in the Milky Way galaxy. III. The total neutral gas disk
journal, November 2015

  • Nakanishi, Hiroyuki; Sofue, Yoshiaki
  • Publications of the Astronomical Society of Japan, Vol. 68, Issue 1
  • DOI: 10.1093/pasj/psv108

A Universal Density Profile from Hierarchical Clustering
journal, December 1997

  • Navarro, Julio F.; Frenk, Carlos S.; White, Simon D. M.
  • The Astrophysical Journal, Vol. 490, Issue 2
  • DOI: 10.1086/304888

A Simple law of star Formation
journal, October 2012


The star Formation rate of Supersonic Magnetohydrodynamic Turbulence
journal, March 2011


H i Velocity Dispersion in NGC 1058
journal, October 2007

  • Petric, A. O.; Rupen, M. P.
  • The Astronomical Journal, Vol. 134, Issue 5
  • DOI: 10.1086/518558

Inefficient star formation: the combined effects of magnetic fields and radiative feedback
journal, September 2009


Scaling Relations of the Properties for co Resolved Structures in Nearby Spiral Galaxies
journal, July 2015


Adiabatic Heating of Contracting Turbulent Fluids
journal, April 2012


Molecular Hydrogen and Global Star Formation Relations in Galaxies
journal, June 2008

  • Robertson, Brant E.; Kravtsov, Andrey V.
  • The Astrophysical Journal, Vol. 680, Issue 2
  • DOI: 10.1086/587796

A Three‐Dimensional Deflagration Model for Type Ia Supernovae Compared with Observations
journal, October 2007

  • Ropke, F. K.; Hillebrandt, W.; Schmidt, W.
  • The Astrophysical Journal, Vol. 668, Issue 2
  • DOI: 10.1086/521347

Effects of Baryons and Dissipation on the Matter Power Spectrum
journal, January 2008

  • Rudd, Douglas H.; Zentner, Andrew R.; Kravtsov, Andrey V.
  • The Astrophysical Journal, Vol. 672, Issue 1
  • DOI: 10.1086/523836

The Rate of Star Formation.
journal, January 1959

  • Schmidt, Maarten
  • The Astrophysical Journal, Vol. 129
  • DOI: 10.1086/146614

The Rate of Star Formation. II. The Rate of Formation of Stars of Different Mass.
journal, February 1963

  • Schmidt, Maarten
  • The Astrophysical Journal, Vol. 137
  • DOI: 10.1086/147553

Numerical Modelling of Astrophysical Turbulence
book, January 2014


Cosmological fluid mechanics with adaptively refined large eddy simulations
journal, April 2014

  • Schmidt, W.; Almgren, A. S.; Braun, H.
  • Monthly Notices of the Royal Astronomical Society, Vol. 440, Issue 4
  • DOI: 10.1093/mnras/stu501

A fluid-dynamical subgrid scale model for highly compressible astrophysical turbulence
journal, March 2011


Star formation and feedback in smoothed particle hydrodynamic simulations – I. Isolated galaxies
journal, November 2006


Making Galaxies In a Cosmological Context: the need for early stellar feedback
journal, October 2012

  • Stinson, G. S.; Brook, C.; Macciò, A. V.
  • Monthly Notices of the Royal Astronomical Society, Vol. 428, Issue 1
  • DOI: 10.1093/mnras/sts028

Dissipation in Compressible Magnetohydrodynamic Turbulence
journal, November 1998

  • Stone, James M.; Ostriker, Eve C.; Gammie, Charles F.
  • The Astrophysical Journal, Vol. 508, Issue 1
  • DOI: 10.1086/311718

What is Driving the h i Velocity Dispersion?
journal, April 2009


The Jeans Condition: A New Constraint on Spatial Resolution in Simulations of Isothermal Self-gravitational Hydrodynamics
journal, November 1997

  • Truelove, J. Kelly; Klein, Richard I.; McKee, Christopher F.
  • The Astrophysical Journal, Vol. 489, Issue 2
  • DOI: 10.1086/310975

Towards the ultimate conservative difference scheme. V. A second-order sequel to Godunov's method
journal, July 1979


Outflow Feedback Regulated Massive star Formation in Parsec-Scale Cluster-Forming Clumps
journal, December 2009


Works referencing / citing this record:

Fast and inefficient star formation due to short-lived molecular clouds and rapid feedback
journal, May 2019

  • Kruijssen, J. M. Diederik; Schruba, Andreas; Chevance, Mélanie
  • Nature, Vol. 569, Issue 7757
  • DOI: 10.1038/s41586-019-1194-3

G.A.S.: I. A prescription for turbulence-regulated star formation and its impact on galaxy properties
journal, July 2019


The [C ii]–SFR correlation in dwarf galaxies across cosmic time
journal, January 2020

  • Lupi, Alessandro; Bovino, Stefano
  • Monthly Notices of the Royal Astronomical Society, Vol. 492, Issue 2
  • DOI: 10.1093/mnras/staa048

What drives gravitational instability in nearby star-forming spirals? The impact of CO and H i velocity dispersions
journal, April 2017

  • Romeo, Alessandro B.; Mogotsi, Keoikantse Moses
  • Monthly Notices of the Royal Astronomical Society, Vol. 469, Issue 1
  • DOI: 10.1093/mnras/stx844

An uncertainty principle for star formation – II. A new method for characterizing the cloud-scale physics of star formation and feedback across cosmic history
journal, May 2018

  • Kruijssen, J. M. Diederik; Schruba, Andreas; Hygate, Alexander P. S.
  • Monthly Notices of the Royal Astronomical Society, Vol. 479, Issue 2
  • DOI: 10.1093/mnras/sty1128

What FIREs up star formation: the emergence of the Kennicutt–Schmidt law from feedback
journal, May 2018

  • Orr, Matthew E.; Hayward, Christopher C.; Hopkins, Philip F.
  • Monthly Notices of the Royal Astronomical Society, Vol. 478, Issue 3
  • DOI: 10.1093/mnras/sty1241

FIRE-2 simulations: physics versus numerics in galaxy formation
journal, June 2018

  • Hopkins, Philip F.; Wetzel, Andrew; Kereš, Dušan
  • Monthly Notices of the Royal Astronomical Society, Vol. 480, Issue 1
  • DOI: 10.1093/mnras/sty1690

Modelling turbulent effects of stellar feedback in cosmological simulations
journal, November 2018

  • Engels, Jan Frederik; Schmidt, Wolfram; Niemeyer, Jens
  • Monthly Notices of the Royal Astronomical Society, Vol. 482, Issue 4
  • DOI: 10.1093/mnras/sty3037

Dynamic localized turbulent diffusion and its impact on the galactic ecosystem
journal, December 2018

  • Rennehan, Douglas; Babul, Arif; Hopkins, Philip F.
  • Monthly Notices of the Royal Astronomical Society, Vol. 483, Issue 3
  • DOI: 10.1093/mnras/sty3376

On the observed diversity of star formation efficiencies in Giant Molecular Clouds
journal, May 2019

  • Grisdale, Kearn; Agertz, Oscar; Renaud, Florent
  • Monthly Notices of the Royal Astronomical Society, Vol. 486, Issue 4
  • DOI: 10.1093/mnras/stz1201

Forming early-type galaxies without AGN feedback: a combination of merger-driven outflows and inefficient star formation
journal, December 2019

  • Kretschmer, Michael; Teyssier, Romain
  • Monthly Notices of the Royal Astronomical Society, Vol. 492, Issue 1
  • DOI: 10.1093/mnras/stz3495

Structure and stability of high-redshift galaxies in cosmological simulations
journal, March 2019

  • Meng, Xi; Gnedin, Oleg Y.; Li, Hui
  • Monthly Notices of the Royal Astronomical Society, Vol. 486, Issue 2
  • DOI: 10.1093/mnras/stz925

Globular cluster formation and evolution in the context of cosmological galaxy assembly: open questions
journal, February 2018

  • Forbes, Duncan A.; Bastian, Nate; Gieles, Mark
  • Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences, Vol. 474, Issue 2210
  • DOI: 10.1098/rspa.2017.0616

The Role of Magnetic Fields in Setting the Star Formation Rate and the Initial Mass Function
journal, February 2019

  • Krumholz, Mark R.; Federrath, Christoph
  • Frontiers in Astronomy and Space Sciences, Vol. 6
  • DOI: 10.3389/fspas.2019.00007

Observational Evidence of Dynamic star Formation rate in Milky way Giant Molecular Clouds
journal, December 2016

  • Lee, Eve J.; Miville-Deschênes, Marc-Antoine; Murray, Norman W.
  • The Astrophysical Journal, Vol. 833, Issue 2
  • DOI: 10.3847/1538-4357/833/2/229

Star Cluster Formation in Cosmological Simulations. i. Properties of Young Clusters
journal, January 2017


On the Appearance of Thresholds in the Dynamical Model of Star Formation
journal, February 2018


Dense Regions in Supersonic Isothermal Turbulence
journal, February 2018


Star Cluster Formation in Cosmological Simulations. II. Effects of Star Formation Efficiency and Stellar Feedback
journal, July 2018

  • Li, Hui; Gnedin, Oleg Y.; Gnedin, Nickolay Y.
  • The Astrophysical Journal, Vol. 861, Issue 2
  • DOI: 10.3847/1538-4357/aac9b8

The Fate of Supernova-heated Gas in Star-forming Regions of the LMC: Lessons for Galaxy Formation?
journal, August 2018

  • Bustard, Chad; Pardy, Stephen A.; D’Onghia, Elena
  • The Astrophysical Journal, Vol. 863, Issue 1
  • DOI: 10.3847/1538-4357/aad08f

What Sets the Slope of the Molecular Kennicutt–Schmidt Relation?
journal, January 2019

  • Semenov, Vadim A.; Kravtsov, Andrey V.; Gnedin, Nickolay Y.
  • The Astrophysical Journal, Vol. 870, Issue 2
  • DOI: 10.3847/1538-4357/aaf163

Dancing in the Dark: Uncertainty in Ultrafaint Dwarf Galaxy Predictions from Cosmological Simulations
journal, March 2019

  • Munshi, Ferah; Brooks, Alyson M.; Christensen, Charlotte
  • The Astrophysical Journal, Vol. 874, Issue 1
  • DOI: 10.3847/1538-4357/ab0085

How Galactic Environment Affects the Dynamical State of Molecular Clouds and Their Star Formation Efficiency
journal, September 2019

  • Schruba, Andreas; Kruijssen, J. M. Diederik; Leroy, Adam K.
  • The Astrophysical Journal, Vol. 883, Issue 1
  • DOI: 10.3847/1538-4357/ab3a43

What FIREs up star formation: the emergence of the Kennicutt–Schmidt law from feedback
text, January 2018

  • Orr, Matthew E.; Hayward, Christopher C.; Hopkins, Philip F.
  • Oxford University Press
  • DOI: 10.5167/uzh-157192

FIRE-2 simulations: physics versus numerics in galaxy formation
text, January 2018

  • Hopkins, Philip F.; Wetzel, Andrew; Kereš, Dušan
  • Oxford University Press
  • DOI: 10.5167/uzh-157191

Observational Evidence of Dynamic Star Formation Rate in Milky Way Giant Molecular Clouds
text, January 2016


The Fate of Supernova-Heated Gas in Star-Forming Regions of the LMC: Lessons for Galaxy Formation?
text, January 2018


The [CII]--SFR correlation in dwarf galaxies across cosmic time
text, January 2019


Fast and inefficient star formation due to short-lived molecular clouds and rapid feedback
text, January 2019