The ALMA-ALPINE [CII] survey: Kennicutt-Schmidt relation in four massive main-sequence galaxies at z ~ 4.5
Artikel i vetenskaplig tidskrift, 2023
Aims. The Kennicutt-Schmidt (KS) relation between the gas and the star formation rate (SFR) surface density (Σgas - ΣSFR) is essential to understand star formation processes in galaxies. To date, it has been measured up to z ~ 2.5 in main-sequence galaxies. In this Letter our aim is to put constraints at z ~ 4.5 using a sample of four massive main-sequence galaxies observed by ALMA at high resolution. Methods. We obtained ~0.3″-resolution [CII] and continuum maps of our objects, which we then converted into gas and obscured SFR surface density maps. In addition, we produced unobscured SFR surface density maps by convolving Hubble ancillary data in the rest-frame UV. We then derived the average ΣSFR in various Σgas bins, and estimated the uncertainties using a Monte Carlo sampling. Results. Our galaxy sample follows the KS relation measured in main-sequence galaxies at lower redshift, and is slightly lower than the predictions from simulations. Our data points probe the high end both in terms of Σgas and ΣSFR, and gas depletion timescales (285-843 Myr) remain similar to z ~ 2 objects. However, three of our objects are clearly morphologically disturbed, and we could have expected shorter gas depletion timescales (≲100 Myr) similar to merger-driven starbursts at lower redshifts. This suggests that the mechanisms triggering starbursts at high redshift may be different than in the low- and intermediate-z Universe.
galaxies: star formation
galaxies: ISM
galaxies: high-redshift
submillimeter: galaxies
Författare
Matthieu Béthermin
Laboratoire d'Astrophysique de Marseille
Observatoire Astronomique de Strasbourg
C. Accard
Observatoire Astronomique de Strasbourg
C. Guillaume
Observatoire Astronomique de Strasbourg
M. Dessauges-Zavadsky
Université de Genève
E. Ibar
Universidad de Valparaíso
P. Cassata
Università di Padova
Istituto nazionale di astrofisica (INAF)
T. Devereaux
Università di Padova
Istituto nazionale di astrofisica (INAF)
A. Faisst
California Institute of Technology (Caltech)
J. Freundlich
Observatoire Astronomique de Strasbourg
G. C. Jones
University of Oxford
K. Kraljic
Observatoire Astronomique de Strasbourg
H. Algera
National Astronomical Observatory of Japan
Hiroshima University
R. O. Amorín
Consejo Nacional de Investigaciones Cientificas y Tecnicas
Universidad de La Serena
S. Bardelli
Istituto nazionale di astrofisica (INAF)
M. Boquien
Universidad de Tarapacá
V. Buat
Laboratoire d'Astrophysique de Marseille
E. Donghia
University of Wisconsin Madison
Y. Dubois
Institut d 'Astrophysique de Paris
Andrea Ferrara
Scuola Normale Superiore di Pisa
Yoshinobu Fudamoto
Chiba University
M. Ginolfi
Osservatorio Astrofisico di Arcetri
Universita degli Studi di Firenze
P. Guillard
Institut d 'Astrophysique de Paris
M. Giavalisco
University of Massachusetts
C. Gruppioni
Istituto nazionale di astrofisica (INAF)
G. Gururajan
Istituto nazionale di astrofisica (INAF)
Universita di Bologna
N. Hathi
Space Telescope Science Institute (STScI)
Christopher C. Hayward
Flatiron Institute
Anton M. Koekemoer
Space Telescope Science Institute (STScI)
Brian C. Lemaux
University of California
Gemini Observatory North
Georgios E. Magdis
Niels Bohr Institute
Cosmic Dawn Center (DAWN)
Danmarks Tekniske Universitet (DTU)
Juan Andrés Molina Tobar
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
D. Narayanan
Cosmic Dawn Center (DAWN)
University of Florida
L. Mayer
Universität Zürich
F. Pozzi
Istituto nazionale di astrofisica (INAF)
F. Rizzo
Niels Bohr Institute
Cosmic Dawn Center (DAWN)
M. Romano
Narodowe Centrum Badan Jadrowych
Istituto nazionale di astrofisica (INAF)
L. Tasca
Laboratoire d'Astrophysique de Marseille
Patrice Theule
Laboratoire d'Astrophysique de Marseille
D. Vergani
Istituto nazionale di astrofisica (INAF)
L. Vallini
Istituto nazionale di astrofisica (INAF)
G. Zamorani
Istituto nazionale di astrofisica (INAF)
A. Zanella
Istituto nazionale di astrofisica (INAF)
E. Zucca
Istituto nazionale di astrofisica (INAF)
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 680 L8Ämneskategorier
Astronomi, astrofysik och kosmologi
Annan fysik
DOI
10.1051/0004-6361/202348115