ALMA constraints on star-forming gas in a prototypical z = 1.5 clumpy galaxy: the dearth of CO(5−4) emission from UV-bright clumps
A. Cibinel(University of Sussex), Tao Wang(National Astronomical Observatory of Japan), D. Elbaz(Université Paris-Saclay), Pierre–Alain Duc(Centre National de la Recherche Scientifique), M. Pannella, E. Le Floc’h(Centrum Badań Kosmicznych), G. Magdis(University of Copenhagen), W. Rujopakarn(Chulalongkorn University), Pascal A. Oesch(University of Geneva), E. Daddi(Centre National de la Recherche Scientifique), P. Jagannathan(National Radio Astronomy Observatory), Kristina Nyland(National Radio Astronomy Observatory), M. Sargent(University of Sussex), Anita Zanella(Osservatorio Astronomico di Padova), F. Bournaud(Direction des Energies), S. Juneau(Institut National de Physique Nucléaire et de Physique des Particules)
Cited by 32
Related Papers
MASS AND ENVIRONMENT AS DRIVERS OF GALAXY EVOLUTION IN SDSS AND zCOSMOS AND THE ORIGIN OF THE SCHECHTER FUNCTION
|The Astrophysical Journal|2010|2k
THE COSMOS2015 CATALOG: EXPLORING THE 1 < z < 6 UNIVERSE WITH HALF A MILLION GALAXIES
|The Astrophysical Journal Supplement Series|2016|1.2k
zCOSMOS: A Large VLT/VIMOS Redshift Survey Covering 0 <<i>z</i>< 3 in the COSMOS Field
|The Astrophysical Journal Supplement Series|2007|1k
High molecular gas fractions in normal massive star-forming galaxies in the young Universe
|Nature|2010|991
A study of the gas-star formation relation over cosmic time★
|Monthly Notices of the Royal Astronomical Society|2010|952