Details

Autor(en) / Beteiligte

• Saintonge, Amélie
• Kauffmann, Guinevere
• Wang, Jing
• Kramer, Carsten
• Tacconi, Linda J.
• Buchbender, Christof
• Catinella, Barbara
• Graciá-Carpio, Javier
• Cortese, Luca
• Fabello, Silvia
• Fu, Jian
• Genzel, Reinhard
• Giovanelli, Riccardo
• Guo, Qi
• Haynes, Martha P.
• Heckman, Timothy M.
• Krumholz, Mark R.
• Lemonias, Jenna
• Li, Cheng
• Moran, Sean
• Rodriguez-Fernandez, Nemesio
• Schiminovich, David
• Schuster, Karl
• Sievers, Albrecht

Titel

COLD GASS, an IRAM legacy survey of molecular gas in massive galaxies - II. The non-universality of the molecular gas depletion time-scale

Ist Teil von

• Monthly notices of the Royal Astronomical Society, 2011-07, Vol.415 (1), p.61-76

Ort / Verlag

Oxford, UK: Blackwell Publishing Ltd

Erscheinungsjahr

2011

Quelle

Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals

Beschreibungen/Notizen

• We study the relation between molecular gas and star formation in a volume-limited sample of 222 galaxies from the COLD GASS survey, with measurements of the CO(1-0) line from the IRAM 30-m telescope. The galaxies are at redshifts 0.025 < z < 0.05 and have stellar masses in the range 10.0 < log M ★/M⊙ < 11.5. The IRAM measurements are complemented by deep Arecibo H i observations and homogeneous Sloan Digital Sky Survey and GALEX photometry. A reference sample that includes both ultraviolet (UV) and far-infrared data is used to calibrate our estimates of star formation rates from the seven optical/UV bands. The mean molecular gas depletion time-scale [ ] for all the galaxies in our sample is 1 Gyr; however, increases by a factor of 6 from a value of ∼0.5 Gyr for galaxies with stellar masses of ∼1010 M⊙ to ∼3 Gyr for galaxies with masses of a few ×1011 M⊙. In contrast, the atomic gas depletion time-scale remains constant at a value of around 3 Gyr. This implies that in high-mass galaxies, molecular and atomic gas depletion time-scales are comparable, but in low-mass galaxies, the molecular gas is being consumed much more quickly than the atomic gas. The strongest dependences of are on the stellar mass of the galaxy [parametrized as ], and on the specific star formation rate (sSFR). A single versus sSFR relation is able to fit both 'normal' star-forming galaxies in our COLD GASS sample and more extreme starburst galaxies (luminous infrared galaxies and ultraluminous infrared galaxies), which have yr. Normal galaxies at z = 1-2 are displaced with respect to the local galaxy population in the versus sSFR plane and have molecular gas depletion times that are a factor of 3-5 times longer at a given value of sSFR due to their significantly larger gas fractions.