GOODS-ALMA: The slow downfall of star formation in z = 2–3 massive galaxies
Authors:
- M. FrancoMFM. Franco
- D. ElbazDED. Elbaz
- L. ZhouLZL. Zhou
- B. MagnelliBMB. Magnelli
- C. SchreiberCSC. Schreiber
- L. CieslaLCL. Ciesla
- M. DickinsonMDM. Dickinson
- N. NagarNNN. Nagar
- G. MagdisGMG. Magdis
- D. M. AlexanderDAD. M. Alexander
- M. BétherminMBM. Béthermin
- R. DemarcoRDR. Demarco
Open Access
- 27 October 2020
- journal article
- research article
- Published by EDP Sciences in Astronomy & Astrophysics
- Vol. 643, A30
Abstract
We investigate the properties of a sample of 35 galaxies, detected with the Atacama Large Millimeter/Submillimeter Array (ALMA) at 1.1 mm in the GOODS-ALMA field (area of 69 arcmin2, resolution = 0.60″, rms ≃ 0.18 mJy beam−1). Using the ultraviolet-to-radio deep multiwavelength coverage of the GOODS–South field, we fit the spectral energy distributions of these galaxies to derive their key physical properties. The galaxies detected by ALMA are among the most massive at z = 2−4 (M⋆, med = 8.5 × 1010 M⊙) and they are either starburst or located in the upper part of the galaxy star-forming main sequence. A significant portion of our galaxy population (∼40%), located at z ∼ 2.5 − 3, exhibits abnormally low gas fractions. The sizes of these galaxies, measured with ALMA, are compatible with the trend between the rest-frame 5000 Å size and stellar mass observed for z ∼ 2 elliptical galaxies, suggesting that they are building compact bulges. We show that there is a strong link between star formation surface density (at 1.1 mm) and gas depletion time: The more compact a galaxy’s star-forming region is, the shorter its lifetime will be (without gas replenishment). The identified compact sources associated with relatively short depletion timescales (∼100 Myr) are the ideal candidates to be the progenitors of compact elliptical galaxies at z ∼ 2.Keywords
All Related Versions
Funding Information
- Science and Technology Facilities Council (ST/R000905/1)
- Deutsche Forschungsgemeinschaft (ID 184018867)
- National Key Research and Development Program of China (2017YFA0402704, 2018YFA0404502)
- National Natural Science Foundation of China (11825302, 11733002, 11773013)
- China Scholarship Council
- Centro de Astrofísica y Tecnologías Afines (AFB-170002)
- Villum Fonden (13160)
- ERC Consolidator Grant funding scheme (648179)
- ERC-StG 'ClustersXCosmo' (71676)
- Science and Technology Facilities Council (ST/P000541/1, ST/T000244/1)
- Programme National Cosmology et Galaxies
This publication has 169 references indexed in Scilit:
- THEORETICAL EVOLUTION OF OPTICAL STRONG LINES ACROSS COSMIC TIMEThe Astrophysical Journal, 2013
- CANDELS: THE PROGENITORS OF COMPACT QUIESCENT GALAXIES ATz∼ 2The Astrophysical Journal, 2013
- Submillimetre galaxies in a hierarchical universe: number counts, redshift distribution and implications for the IMFMonthly Notices of the Royal Astronomical Society, 2012
- CANDELS: THE COSMIC ASSEMBLY NEAR-INFRARED DEEP EXTRAGALACTIC LEGACY SURVEY—THE HUBBLE SPACE TELESCOPE OBSERVATIONS, IMAGING DATA PRODUCTS, AND MOSAICSThe Astrophysical Journal Supplement Series, 2011
- CANDELS: THE COSMIC ASSEMBLY NEAR-INFRARED DEEP EXTRAGALACTIC LEGACY SURVEYThe Astrophysical Journal Supplement Series, 2011
- GOODS- HERSCHEL : GAS-TO-DUST MASS RATIOS AND CO-TO-H 2 CONVERSION FACTORS IN NORMAL AND STARBURSTING GALAXIES AT HIGH- zThe Astrophysical Journal Letters, 2011
- GOODS–Herschel: an infrared main sequence for star-forming galaxiesAstronomy & Astrophysics, 2011
- THE CO-TO-H2CONVERSION FACTOR FROM INFRARED DUST EMISSION ACROSS THE LOCAL GROUPThe Astrophysical Journal, 2011
- DEEP U BAND AND R IMAGING OF GOODS-SOUTH: OBSERVATIONS, DATA REDUCTION AND FIRST RESULTS,The Astrophysical Journal Supplement Series, 2009
- The Nature of Compact Galaxies in the Hubble Deep Field. II. Spectroscopic Properties and Implications for the Evolution of the Star Formation Rate Density of the UniverseThe Astrophysical Journal, 1997