Galaxy metallicities depend primarily on stellar mass and molecular gas mass
Authors:
- M. S. BothwellMBM. S. Bothwell
- R. MaiolinoRMR. Maiolino
- C. CiconeCCC. Cicone
- Y. PengYPY. Peng
- J. WaggJWJ. Wagg
- 26 October 2016
- journal article
- Published by EDP Sciences in Astronomy & Astrophysics
- Vol. 595, A48
Abstract
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysicsKeywords
All Related Versions
This publication has 32 references indexed in Scilit:
- Molecular gas as the driver of fundamental galactic relationsMonthly Notices of the Royal Astronomical Society, 2015
- ALLSMOG: an APEX Low-redshift Legacy Survey for MOlecular Gas – I. Molecular gas scaling relations, and the effect of the CO/H2 conversion factorMonthly Notices of the Royal Astronomical Society, 2014
- The neutral hydrogen content of galaxies in cosmological hydrodynamic simulationsMonthly Notices of the Royal Astronomical Society, 2013
- A fundamental relation between the metallicity, gas content and stellar mass of local galaxiesMonthly Notices of the Royal Astronomical Society, 2013
- The physics of the fundamental metallicity relationMonthly Notices of the Royal Astronomical Society, 2013
- A survey of molecular gas in luminous sub-millimetre galaxiesMonthly Notices of the Royal Astronomical Society, 2013
- The Herschel Reference SurveyPublications of the Astronomical Society of the Pacific, 2010
- A Redshift Survey of the Submillimeter Galaxy PopulationThe Astrophysical Journal, 2005
- Galactic Stellar and Substellar Initial Mass FunctionPublications of the Astronomical Society of the Pacific, 2003
- Stellar Mass‐to‐Light Ratios and the Tully‐Fisher RelationThe Astrophysical Journal, 2001