SDSS-IV MaNGA: How the Stellar Populations of Passive Central Galaxies Depend on Stellar and Halo Mass
Abstract
We analyze spatially resolved and co-added SDSS-IV MaNGA spectra with signal-to-noise ratio ~100 from 2200 passive central galaxies (z ~ 0.05) to understand how central galaxy assembly depends on stellar mass (M*) and halo mass (Mh). We control for systematic errors in Mh by employing a new group catalog from Tinker and the widely used Yang et al. catalog. At fixed M*, the strengths of several stellar absorption features vary systematically with Mh. Completely model-free, this is one of the first indications that the stellar populations of centrals with identical M* are affected by the properties of their host halos. To interpret these variations, we applied full spectral fitting with the code alf. At fixed M*, centrals in more massive halos are older, show lower [Fe/H], and have higher [Mg/Fe] with 3.5σ confidence. We conclude that halos not only dictate how much M* galaxies assemble but also modulate their chemical enrichment histories. Turning to our analysis at fixed Mh, high-M* centrals are older, show lower [Fe/H], and have higher [Mg/Fe] for Mh > 1012 h–1 M⊙ with confidence >4σ. While massive passive galaxies are thought to form early and rapidly, our results are among the first to distinguish these trendsmore »
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[4];
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- Univ. of California, Santa Cruz, CA (United States)
- New York Univ. (NYU), NY (United States)
- Istituto Nazionale di Astrofisica (INAF), Firenze (Italy)
- Pontifica Universidad Catolica de Valparaíso (Chile)
- Chinese Academy of Sciences (CAS) (China)
- Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
- Haverford College, PA (United States)
- Univ. of North Carolina, Asheville, NC (United States)
- Space Telescope Science Institute, Baltimore, MD (United States)
- Macquarie Univ., NSW (Australia)
- Univ. of Nottingham (United Kingdom)
- Max Planck Inst. fuer Extraterrestrische Physik, Garching (Germany)
- Univ. of Kentucky, Lexington, KY (United States)
- Univ. of Wisconsin, Madison, WI (United States); South African Astronomical Observatory, Cape Town (South Africa); Univ. of Cape Town (South Africa)
- Univ. Nacional Autonoma de Mexico (UNAM), Mexico City (Mexico)
- Univ. of Pittsburgh, PA (United States)
- Universidad Católica del Norte (Chile)
- Bernardo O'Higgins University (Chile)
- Apache Point Observatory, Sunspot, NM (United States)
- Univ. of St. Andrews, Scotland (United Kingdom)
- Universidad de Atacama (Chile); Pontifica Universidad Catolica de Chile (Chile)
- Univ. of Utah, Salt Lake City, UT (United States)
- Univ. of Texas, Austin, TX (United States)
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- OSTI Identifier:
- 1905505
- Grant/Contract Number:
- AC02-05CH11231
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal
- Additional Journal Information:
- Journal Volume: 933; Journal Issue: 1; Journal ID: ISSN 0004-637X
- Publisher:
- IOP Publishing
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; early-type galaxies; elliptical galaxies; galaxies; galaxy ages; galaxy evolution; galaxy stellar content; quenched galaxies; galaxy abundances; galaxy dark matter halos; galaxy environments; galaxy properties; galaxy spectroscopy
Citation Formats
Oyarzún, Grecco A., Bundy, Kevin, Westfall, Kyle B., Tinker, Jeremy L., Belfiore, Francesco, Argudo-Fernández, Maria, Zheng, Zheng, Conroy, Charlie, Masters, Karen L., Wake, David, Law, David R., McDermid, Richard M., Aragón-Salamanca, Alfonso, Parikh, Taniya, Yan, Renbin, Bershady, Matthew, Sánchez, Sebastián F., Andrews, Brett H., Fernández-Trincado, José G., Lane, Richard R., Bizyaev, D., Boardman, Nicholas Fraser, Lacerna, Ivan, Brownstein, J. R., Drory, Niv, and Zhang, Kai. SDSS-IV MaNGA: How the Stellar Populations of Passive Central Galaxies Depend on Stellar and Halo Mass. United States: N. p., 2022.
Web. doi:10.3847/1538-4357/ac7048.
Oyarzún, Grecco A., Bundy, Kevin, Westfall, Kyle B., Tinker, Jeremy L., Belfiore, Francesco, Argudo-Fernández, Maria, Zheng, Zheng, Conroy, Charlie, Masters, Karen L., Wake, David, Law, David R., McDermid, Richard M., Aragón-Salamanca, Alfonso, Parikh, Taniya, Yan, Renbin, Bershady, Matthew, Sánchez, Sebastián F., Andrews, Brett H., Fernández-Trincado, José G., Lane, Richard R., Bizyaev, D., Boardman, Nicholas Fraser, Lacerna, Ivan, Brownstein, J. R., Drory, Niv, & Zhang, Kai. SDSS-IV MaNGA: How the Stellar Populations of Passive Central Galaxies Depend on Stellar and Halo Mass. United States. https://doi.org/10.3847/1538-4357/ac7048
Oyarzún, Grecco A., Bundy, Kevin, Westfall, Kyle B., Tinker, Jeremy L., Belfiore, Francesco, Argudo-Fernández, Maria, Zheng, Zheng, Conroy, Charlie, Masters, Karen L., Wake, David, Law, David R., McDermid, Richard M., Aragón-Salamanca, Alfonso, Parikh, Taniya, Yan, Renbin, Bershady, Matthew, Sánchez, Sebastián F., Andrews, Brett H., Fernández-Trincado, José G., Lane, Richard R., Bizyaev, D., Boardman, Nicholas Fraser, Lacerna, Ivan, Brownstein, J. R., Drory, Niv, and Zhang, Kai. Wed .
"SDSS-IV MaNGA: How the Stellar Populations of Passive Central Galaxies Depend on Stellar and Halo Mass". United States. https://doi.org/10.3847/1538-4357/ac7048. https://www.osti.gov/servlets/purl/1905505.
@article{osti_1905505,
title = {SDSS-IV MaNGA: How the Stellar Populations of Passive Central Galaxies Depend on Stellar and Halo Mass},
author = {Oyarzún, Grecco A. and Bundy, Kevin and Westfall, Kyle B. and Tinker, Jeremy L. and Belfiore, Francesco and Argudo-Fernández, Maria and Zheng, Zheng and Conroy, Charlie and Masters, Karen L. and Wake, David and Law, David R. and McDermid, Richard M. and Aragón-Salamanca, Alfonso and Parikh, Taniya and Yan, Renbin and Bershady, Matthew and Sánchez, Sebastián F. and Andrews, Brett H. and Fernández-Trincado, José G. and Lane, Richard R. and Bizyaev, D. and Boardman, Nicholas Fraser and Lacerna, Ivan and Brownstein, J. R. and Drory, Niv and Zhang, Kai},
abstractNote = {We analyze spatially resolved and co-added SDSS-IV MaNGA spectra with signal-to-noise ratio ~100 from 2200 passive central galaxies (z ~ 0.05) to understand how central galaxy assembly depends on stellar mass (M*) and halo mass (Mh). We control for systematic errors in Mh by employing a new group catalog from Tinker and the widely used Yang et al. catalog. At fixed M*, the strengths of several stellar absorption features vary systematically with Mh. Completely model-free, this is one of the first indications that the stellar populations of centrals with identical M* are affected by the properties of their host halos. To interpret these variations, we applied full spectral fitting with the code alf. At fixed M*, centrals in more massive halos are older, show lower [Fe/H], and have higher [Mg/Fe] with 3.5σ confidence. We conclude that halos not only dictate how much M* galaxies assemble but also modulate their chemical enrichment histories. Turning to our analysis at fixed Mh, high-M* centrals are older, show lower [Fe/H], and have higher [Mg/Fe] for Mh > 1012 h–1 M⊙ with confidence >4σ. While massive passive galaxies are thought to form early and rapidly, our results are among the first to distinguish these trends at fixed Mh. They suggest that high-M* centrals experienced unique early formation histories, either through enhanced collapse and gas fueling or because their halos were early forming and highly concentrated, a possible signal of galaxy assembly bias.},
doi = {10.3847/1538-4357/ac7048},
journal = {The Astrophysical Journal},
number = 1,
volume = 933,
place = {United States},
year = {Wed Jul 06 00:00:00 EDT 2022},
month = {Wed Jul 06 00:00:00 EDT 2022}
}
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