Low-energy Population III supernovae and the origin of extremely metal-poor stars

Chen, Ke-Jung; Heger, Alexander; Whalen, Daniel J.; Moriya, Takashi J.; Bromm, Volker; Woosley, S. E.

doi:10.1093/mnras/stx470

Title: Low-energy Population III supernovae and the origin of extremely metal-poor stars

Journal Article · Thu Feb 23 00:00:00 EST 2017 · Monthly Notices of the Royal Astronomical Society

DOI:https://doi.org/10.1093/mnras/stx470· OSTI ID:1523829

Chen, Ke-Jung ^[1]; Heger, Alexander ^[2]; Whalen, Daniel J. ^[3]; Moriya, Takashi J. ^[4]; Bromm, Volker ^[5]; Woosley, S. E. ^[6]

National Astronomical Observatory of Japan, Tokyo (Japan); Academia Sinica, Taipei (Taiwan); Univ. of California, Santa Cruz, CA (United States)
Univ. of Minnesota, Minneapolis, MN (United States); Monash Univ., Melbourne, VIC (Australia); Univ. of Notre Dame, IN (United States)
Portsmouth Univ. (United Kingdom)
National Astronomical Observatory of Japan, Tokyo (Japan)
Univ. of Texas, Austin, TX (United States)
Univ. of California, Santa Cruz, CA (United States)

Some ancient, dim, metal-poor stars may have formed in the ashes of the first supernovae (SNe). If their chemical abundances can be reconciled with the elemental yields of specific Population III (Pop III) explosions, they could reveal the properties of primordial stars. But multidimensional simulations of such explosions are needed to predict their yields because dynamical instabilities can dredge material up from deep in the ejecta that would otherwise be predicted to fall back on to the central remnant and be lost in one-dimensional (1D) models. We have performed two-dimensional (2D) numerical simulations of two low-energy Pop III SNe, a 12.4 M_⊙ explosion and a 60 M_⊙ explosion, and find that they produce elemental yields that are a good fit to those measured in the most iron-poor star discovered to date, SMSS J031300.36-670839.3 (J031300). Fallback on to the compact remnant in these weak explosions accounts for the lack of measurable iron in J031300 and its low iron-group abundances in general. Our 2D explosions produce higher abundances of heavy elements (atomic number Z > 20) than their 1D counterparts due to dredge-up by fluid instabilities. Since almost no ⁵⁶Ni is ejected by these weak SNe, their low luminosities will prevent their detection in the near-infrared with the James Webb Space Telescope and future 30-m telescopes on the ground. The only evidence that they ever occurred will remain in the fossil abundance record

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Research Organization:: Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)

Sponsoring Organization:: USDOE Office of Science (SC)

Grant/Contract Number:: SC0010676; AC02-05CH11231; FC02-09ER41618

OSTI ID:: 1523829

Journal Information:: Monthly Notices of the Royal Astronomical Society, Vol. 467, Issue 4; ISSN 0035-8711

Publisher:: Royal Astronomical SocietyCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 17 works

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Faint Population iii Supernovae as the Origin of the most Iron-Poor Stars Ishigaki, Miho N.; Tominaga, Nozomu; Kobayashi, Chiaki The Astrophysical Journal, Vol. 792, Issue 2 https://doi.org/10.1088/2041-8205/792/2/L32	journal	August 2014
FINDING THE FIRST COSMIC EXPLOSIONS. IV. 90–140 $\;{{M}_{\odot }}$ PAIR-INSTABILITY SUPERNOVAE Smidt, Joseph; Whalen, Daniel J.; Chatzopoulos, E. The Astrophysical Journal, Vol. 805, Issue 1 https://doi.org/10.1088/0004-637X/805/1/44	journal	May 2015
Simulations on a Moving Mesh: the Clustered Formation of Population iii Protostars Greif, Thomas H.; Springel, Volker; White, Simon D. M. The Astrophysical Journal, Vol. 737, Issue 2 https://doi.org/10.1088/0004-637X/737/2/75	journal	August 2011
Lower Metal Enrichment of Virialized Gas in Minihalos Cen, Renyue; Riquelme, Mario A. The Astrophysical Journal, Vol. 674, Issue 2 https://doi.org/10.1086/524724	journal	February 2008
Pair Instability Supernovae: Light Curves, Spectra, and Shock Breakout Kasen, Daniel; Woosley, S. E.; Heger, Alexander The Astrophysical Journal, Vol. 734, Issue 2 https://doi.org/10.1088/0004-637X/734/2/102	journal	June 2011
A new statistical model for Population III supernova rates: discriminating between ΛCDM and WDM cosmologies Magg, Mattis; Hartwig, Tilman; Glover, Simon C. O. Monthly Notices of the Royal Astronomical Society, Vol. 462, Issue 4 https://doi.org/10.1093/mnras/stw1882	journal	July 2016
SEEING THE FIRST SUPERNOVAE AT THE EDGE OF THE UNIVERSE WITH JWST Whalen, Daniel J.; Fryer, Chris L.; Holz, Daniel E. The Astrophysical Journal, Vol. 762, Issue 1 https://doi.org/10.1088/2041-8205/762/1/L6	journal	December 2012

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Metal-poor star formation triggered by the feedback effects from Pop III stars Chiaki, Gen; Susa, Hajime; Hirano, Shingo Monthly Notices of the Royal Astronomical Society, Vol. 475, Issue 4 https://doi.org/10.1093/mnras/sty040	journal	February 2018
Descendants of the first stars: the distinct chemical signature of second-generation stars Hartwig, Tilman; Yoshida, Naoki; Magg, Mattis Monthly Notices of the Royal Astronomical Society, Vol. 478, Issue 2 https://doi.org/10.1093/mnras/sty1176	journal	May 2018
Fingerprint of the first stars: multi-enriched extremely metal-poor stars in the TOPoS survey Hartwig, Tilman; Ishigaki, Miho N.; Klessen, Ralf S. Monthly Notices of the Royal Astronomical Society, Vol. 482, Issue 1 https://doi.org/10.1093/mnras/sty2783	journal	October 2018
Detecting strongly lensed supernovae at z ∼ 5–7 with LSST Rydberg, Claes-Erik; Whalen, Daniel J.; Maturi, Matteo Monthly Notices of the Royal Astronomical Society, Vol. 491, Issue 2 https://doi.org/10.1093/mnras/stz3203	journal	November 2019
The Initial Mass Function of the First Stars Inferred from Extremely Metal-poor Stars Ishigaki, Miho N.; Tominaga, Nozomu; Kobayashi, Chiaki The Astrophysical Journal, Vol. 857, Issue 1 https://doi.org/10.3847/1538-4357/aab3de	journal	April 2018
Radiation Hydrodynamical Simulations of the First Quasars Smidt, Joseph; Whalen, Daniel J.; Johnson, Jarrett L. The Astrophysical Journal, Vol. 865, Issue 2 https://doi.org/10.3847/1538-4357/aad7b8	journal	September 2018
Fallback Accretion-powered Supernova Light Curves Based on a Neutrino-driven Explosion Simulation of a 40 M ⊙ Star Moriya, Takashi J.; Müller, Bernhard; Chan, Conrad The Astrophysical Journal, Vol. 880, Issue 1 https://doi.org/10.3847/1538-4357/ab2643	journal	July 2019
Black Hole Formation and Fallback during the Supernova Explosion of a 40 M _⊙ Star Chan, Conrad; Müller, Bernhard; Heger, Alexander The Astrophysical Journal, Vol. 852, Issue 1 https://doi.org/10.3847/2041-8213/aaa28c	journal	January 2018
Metal-poor star formation triggered by the feedback effects from Pop III stars Chiaki, Gen; Susa, Hajime; Hirano, Shingo arXiv https://doi.org/10.48550/arxiv.1801.01583	text	January 2018
Fingerprint of the first stars: multi-enriched extremely metal-poor stars in the TOPoS survey Hartwig, Tilman; Ishigaki, Miho N.; Klessen, Ralf S. arXiv https://doi.org/10.48550/arxiv.1810.04713	text	January 2018

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Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
hydrodynamics
instabilities
stars: early-type
stars: Population III
supe-rnovae: general
cosmology: theory