How do central and satellite galaxies quench? – Insights from spatially resolved spectroscopy in the MaNGA survey
Abstract
ABSTRACT We investigate how star formation quenching proceeds within central and satellite galaxies using spatially resolved spectroscopy from the SDSS-IV MaNGA DR15. We adopt a complete sample of star formation rate surface densities (ΣSFR), derived in Bluck et al. (2020), to compute the distance at which each spaxel resides from the resolved star forming main sequence (ΣSFR − Σ* relation): ΔΣSFR. We study galaxy radial profiles in ΔΣSFR, and luminosity weighted stellar age (AgeL), split by a variety of intrinsic and environmental parameters. Via several statistical analyses, we establish that the quenching of central galaxies is governed by intrinsic parameters, with central velocity dispersion (σc) being the most important single parameter. High mass satellites quench in a very similar manner to centrals. Conversely, low mass satellite quenching is governed primarily by environmental parameters, with local galaxy overdensity (δ5) being the most important single parameter. Utilizing the empirical MBH − σc relation, we estimate that quenching via AGN feedback must occur at $$M_{\rm BH} \ge 10^{6.5-7.5} \, \mathrm{M}_{\odot }$$, and is marked by steeply rising ΔΣSFR radial profiles in the green valley, indicating ‘inside-out’ quenching. On the other hand, environmental quenching occurs at overdensities of 10–30 times the average galaxy density at z∼ 0.1, and is marked by steeply declining ΔΣSFR profiles, indicating ‘outside-in’ quenching. Finally, through an analysis of stellar metallicities, we conclude that both intrinsic and environmental quenching must incorporate significant starvation of gas supply.
- Authors:
-
[1];
[1];
[2];
[2];
[5];
- Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK, Cavendish Laboratory – Astrophysics Group, University of Cambridge, 19 JJ Thomson Avenue, Cambridge CB3 0HE, UK
- Department of Physics and Astronomy, University of Victoria, Finnerty Road, Victoria, British Columbia V8P 1A1, Canada
- Instituto de Astronomia, Universidad Nacional Autonoma de Mexico, A. P. 70-264, C.P. 04510 Mexico, D.F., Mexico
- NRC Herzberg Astronomy and Astrophysics, 5071 West Saanich Road, Victoria, British Columbia V9E 2E7, Canada
- Department of Physics and Astronomy, Pomona College, Claremont, CA 91711, USA
- Centre for Astronomy and Particle Theory, University of Nottingham, University Park, Nottingham NG7 2RD, UK
- Publication Date:
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1670812
- Resource Type:
- Published Article
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Name: Monthly Notices of the Royal Astronomical Society Journal Volume: 499 Journal Issue: 1; Journal ID: ISSN 0035-8711
- Publisher:
- Oxford University Press
- Country of Publication:
- United Kingdom
- Language:
- English
Citation Formats
Bluck, Asa F. L., Maiolino, Roberto, Piotrowska, Joanna M., Trussler, James, Ellison, Sara L., Sánchez, Sebastian F., Thorp, Mallory D., Teimoorinia, Hossen, Moreno, Jorge, and Conselice, Christopher J.. How do central and satellite galaxies quench? – Insights from spatially resolved spectroscopy in the MaNGA survey. United Kingdom: N. p., 2020.
Web. doi:10.1093/mnras/staa2806.
Bluck, Asa F. L., Maiolino, Roberto, Piotrowska, Joanna M., Trussler, James, Ellison, Sara L., Sánchez, Sebastian F., Thorp, Mallory D., Teimoorinia, Hossen, Moreno, Jorge, & Conselice, Christopher J.. How do central and satellite galaxies quench? – Insights from spatially resolved spectroscopy in the MaNGA survey. United Kingdom. https://doi.org/10.1093/mnras/staa2806
Bluck, Asa F. L., Maiolino, Roberto, Piotrowska, Joanna M., Trussler, James, Ellison, Sara L., Sánchez, Sebastian F., Thorp, Mallory D., Teimoorinia, Hossen, Moreno, Jorge, and Conselice, Christopher J.. Tue .
"How do central and satellite galaxies quench? – Insights from spatially resolved spectroscopy in the MaNGA survey". United Kingdom. https://doi.org/10.1093/mnras/staa2806.
@article{osti_1670812,
title = {How do central and satellite galaxies quench? – Insights from spatially resolved spectroscopy in the MaNGA survey},
author = {Bluck, Asa F. L. and Maiolino, Roberto and Piotrowska, Joanna M. and Trussler, James and Ellison, Sara L. and Sánchez, Sebastian F. and Thorp, Mallory D. and Teimoorinia, Hossen and Moreno, Jorge and Conselice, Christopher J.},
abstractNote = {ABSTRACT We investigate how star formation quenching proceeds within central and satellite galaxies using spatially resolved spectroscopy from the SDSS-IV MaNGA DR15. We adopt a complete sample of star formation rate surface densities (ΣSFR), derived in Bluck et al. (2020), to compute the distance at which each spaxel resides from the resolved star forming main sequence (ΣSFR − Σ* relation): ΔΣSFR. We study galaxy radial profiles in ΔΣSFR, and luminosity weighted stellar age (AgeL), split by a variety of intrinsic and environmental parameters. Via several statistical analyses, we establish that the quenching of central galaxies is governed by intrinsic parameters, with central velocity dispersion (σc) being the most important single parameter. High mass satellites quench in a very similar manner to centrals. Conversely, low mass satellite quenching is governed primarily by environmental parameters, with local galaxy overdensity (δ5) being the most important single parameter. Utilizing the empirical MBH − σc relation, we estimate that quenching via AGN feedback must occur at $M_{\rm BH} \ge 10^{6.5-7.5} \, \mathrm{M}_{\odot }$, and is marked by steeply rising ΔΣSFR radial profiles in the green valley, indicating ‘inside-out’ quenching. On the other hand, environmental quenching occurs at overdensities of 10–30 times the average galaxy density at z∼ 0.1, and is marked by steeply declining ΔΣSFR profiles, indicating ‘outside-in’ quenching. Finally, through an analysis of stellar metallicities, we conclude that both intrinsic and environmental quenching must incorporate significant starvation of gas supply.},
doi = {10.1093/mnras/staa2806},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 1,
volume = 499,
place = {United Kingdom},
year = {2020},
month = {9}
}
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