Molecular gas and dust properties of galaxies from the Great Observatories All-sky LIRG Survey

@article{HerreroIllana2019MolecularGA,
  title={Molecular gas and dust properties of galaxies from the Great Observatories All-sky LIRG Survey},
  author={Rub{\'e}n Herrero-Illana and George C. Privon and Aaron S. Evans and Tanio D'iaz-Santos and Miguel 'Angel P'erez-Torres and U V. and A. Alberdi and Kazushi Iwasawa and Lee Armus and Susanne Aalto and Joseph M. Mazzarella and Jason K. Chu and David B. Sanders and L. Barcos-Mu{\~n}oz and Vassilis Charmandaris and Sean T. Linden and Ilsang Yoon and David T. Frayer and Hanae Inami and D.-C. Kim and H. Jacob Borish and J. Conway and Eric J. Murphy and Y. Song and Sabrina Stierwalt and Jason Surace},
  journal={Astronomy \& Astrophysics},
  year={2019}
}
We present IRAM-30 m Telescope 12CO and 13CO observations of a sample of 55 luminous and ultraluminous infrared galaxies (LIRGs and ULIRGs) in the local universe. This sample is a subset of the Great Observatory All-Sky LIRG Survey (GOALS), for which we use ancillary multi-wavelength data to better understand their interstellar medium and star formation properties. Fifty-three (96%) of the galaxies are detected in 12CO, and 29 (52%) are also detected in 13CO above a 3σ level. The median full… Expand
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A hard X-ray view of luminous and ultra-luminous infrared galaxies in GOALS – I. AGN obscuration along the merger sequence
  • C. Ricci, G. Privon, +25 authors S Yamada
  • Physics
  • Monthly Notices of the Royal Astronomical Society
  • 2021
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References

SHOWING 1-10 OF 76 REFERENCES
THE GREAT OBSERVATORIES ALL-SKY LIRG SURVEY: COMPARISON OF ULTRAVIOLET AND FAR-INFRARED PROPERTIES
The Great Observatories All-sky LIRG Survey (GOALS) consists of a complete sample of 202 luminous infrared galaxies (LIRGs) selected from the IRAS Revised Bright Galaxy Sample (RBGS). The galaxiesExpand
Mid-infrared Properties of Luminous Infrared Galaxies. II. Probing the Dust and Gas Physics of the GOALS Sample
The Great Observatories All-sky LIRG Survey (GOALS) is a comprehensive, multiwavelength study of luminous infrared galaxies (LIRGs) in the local universe. Here, we present the results of aExpand
Cold Molecular Gas Along the Merger Sequence in Local Luminous Infrared Galaxies
We present an initial result from the 12CO (J=1-0) survey of 79 galaxies in 62 local luminous and ultra-luminous infrared galaxy (LIRG and ULIRG) systems obtained using the 45 m telescope at theExpand
C-GOALS: Chandra observations of a complete sample of luminous infrared galaxies from the IRAS Revised Bright Galaxy Survey
We present X-ray data for a complete sample of 44 luminous infrared galaxies (LIRGs), obtained with the Chandra X-ray Observatory. These are the X-ray observations of the high luminosity portion ofExpand
LUMINOUS INFRARED GALAXIES WITH THE SUBMILLIMETER ARRAY. I. SURVEY OVERVIEW AND THE CENTRAL GAS TO DUST RATIO
We present new data obtained with the Submillimeter Array for a sample of 14 nearby luminous and ultraluminous infrared galaxies. The galaxies were selected to have distances D_L 11.4. The galaxiesExpand
CO Molecular Gas in Infrared-luminous Galaxies
We present the first statistical survey of the properties of the 12CO(1-0) and 12CO(3-2) line emission from the nuclei of a nearly complete subsample of 60 infrared (IR) luminous galaxies selectedExpand
The Nuclear Structure in Nearby Luminous Infrared Galaxies: HST NICMOS Imaging of the GOALS Sample
We present results of Hubble Space Telescope NICMOS H-band imaging of 73 of most luminous (i.e., log[L_IR/L_0]>11.4) Infrared Galaxies (LIRGs) in the Great Observatories All-sky LIRG Survey (GOALS).Expand
THE MOLECULAR INTERSTELLAR MEDIUM IN ULTRALUMINOUS INFRARED GALAXIES
We present observations with the IRAM 30 m telescope of CO in a large sample of ultraluminous IR galaxies out to redshift z = 0.3. Most of the ultraluminous galaxies in this sample are interacting,Expand
Molecular gas in luminous infrared galaxies
Radio observations of 60 bright IRAS galaxies with redshifts of 1500-25,000 km/sec are reported. Data obtained in the 1-0 line of CO using the 12-m NRAO radio telescope during 1985-1988 are presentedExpand
GOALS: The Great Observatories All-Sky LIRG Survey
ABSTRACT.The Great Observatories All-Sky LIRG Survey (GOALS20) combines data from NASA’s Spitzer Space Telescope, Chandra X-Ray Observatory, Hubble Space Telescope (HST), and Galaxy EvolutionExpand
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