Highest Redshift Image of Neutral Hydrogen in Emission: A CHILES Detection of a Starbursting Galaxy at z = 0.376

Autor: Jay Strader, R. Salinas, Kathryn Kreckel, Julia Gross, Christopher A. Hales, Richard Dodson, Ximena Fernández, J. H. van Gorkom, Andreas Wicenec, Daniel J. Pisano, Natasha Maddox, Jennifer Donovan Meyer, Marc Verheijen, Evangelia Tremou, R. Chávez, Attila Popping, Martin Meyer, Lucas Hunt, D. M. Lucero, Min S. Yun, K. Golap, Aeree Chung, Emmanuel Momjian, Patricia A. Henning, Matthew A. Bershady, Yara L. Jaffé, Monica Sanchez-Barrantes, David Schiminovich, John E. Hibbard, Kelley M. Hess, Nick Scoville, Eric M. Wilcots, Tom Oosterloo, Laura Chomiuk, Hansung B. Gim
Přispěvatelé: Astronomy
Jazyk: angličtina
Rok vydání: 2016
Předmět:
Zdroj: The Astrophysical Journal, 824(1):L1. IOP PUBLISHING LTD
ISSN: 0004-637X
Popis: Our current understanding of galaxy evolution still has many uncertainties associated with the details of accretion, processing, and removal of gas across cosmic time. The next generation of radio telescopes will image the neutral hydrogen (HI) in galaxies over large volumes at high redshifts, which will provide key insights into these processes. We are conducting the COSMOS HI Large Extragalactic Survey (CHILES) with the Karl G. Jansky Very Large Array, which is the first survey to simultaneously observe HI from z=0 to z~0.5. Here, we report the highest redshift HI 21-cm detection in emission to date of the luminous infrared galaxy (LIRG) COSMOS J100054.83+023126.2 at z=0.376 with the first 178 hours of CHILES data. The total HI mass is $(2.9\pm1.0)\times10^{10}~M_\odot$, and the spatial distribution is asymmetric and extends beyond the galaxy. While optically the galaxy looks undisturbed, the HI distribution suggests an interaction with candidate a candidate companion. In addition, we present follow-up Large Millimeter Telescope CO observations that show it is rich in molecular hydrogen, with a range of possible masses of $(1.8-9.9)\times10^{10}~M_\odot$. This is the first study of the HI and CO in emission for a single galaxy beyond z~0.2.
7 pages, 5 figures, accepted for publication in ApJL
Databáze: OpenAIRE