Home News About Us Contact Contributors Disclaimer Privacy Policy Help FAQ

Home
Search
Quick Search
Advanced
Fulltext
Browse
Collections
Persons
My eDoc
Session History
Login
Name:
Password:
Documentation
Help
Support Wiki
Direct access to
document ID:


          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



ID: 730054.0, MPI für Astronomie / Publikationen_mpia
The inferred evolution of the cold gas properties of CANDELS galaxies at 0.5 < z < 3.0
Authors:Popping, G.; Caputi, K. I.; Trager, S. C.; Somerville, R. S.; Dekel, A.; Kassin, S. A.; Kocevski, D. D.; Koekemoer, A. M.; Faber, S. M.; Ferguson, H. C.; Galametz, A.; Grogin, N. A.; Guo, Y.; Lu, Y.; Wel, A. v. d.; Weiner, B. J.
Date of Publication (YYYY-MM-DD):2015
Title of Journal:Monthly Notices of the Royal Astronomical Society
Volume:454
Start Page:2258
End Page:2276
Audience:Not Specified
Abstract / Description:We derive the total cold gas, atomic hydrogen, and molecular gas masses of approximately 24 000 galaxies covering four decades in stellar mass at redshifts 0.5 < z < 3.0, taken from the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey survey. Our inferences are based on the inversion of a molecular hydrogen based star formation law, coupled with a prescription to separate atomic and molecular gas. We find that: (1) there is an increasing trend between the inferred cold gas (H I and H2), H I, and H2 mass and the stellar mass of galaxies down to stellar masses of 108 M already in place at z = 3; (2) the molecular fractions of cold gas increase with increasing stellar mass and look-back time; (3) there is hardly any evolution in the mean H I content of galaxies at fixed stellar mass; (4) the cold gas fraction and relative amount of molecular hydrogen in galaxies decrease at a relatively constant rate with time, independent of stellar mass; (5) there is a large population of low stellar mass galaxies dominated by atomic gas. These galaxies are very gas rich, but only a minor fraction of their gas is molecular; 6) the ratio between star formation rate (SFR) and inferred total cold gas mass (H I + H2) of galaxies (i.e. star formation efficiency; SFE) increases with star formation at fixed stellar masses. Due to its simplicity, the presented approach is valuable to assess the impact of selection biases on small samples of directly observed gas masses and to extend scaling relations down to stellar mass ranges and redshifts that are currently difficult to probe with direct measurements of gas content.
Free Keywords:ISM: molecules; galaxies: evolution; galaxies: formation; galaxies: ISM
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:ISSN:0035-8711
URL:http://cdsads.u-strasbg.fr/abs/2015MNRAS.454.2258P
The scope and number of records on eDoc is subject to the collection policies defined by each institute - see "info" button in the collection browse view.