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Published March 2, 2001 | Published + Submitted
Journal Article Open

H I line observations of luminous infrared galaxy mergers

Abstract

A total of 19 luminous infrared galaxy mergers, with L_(IR) ≳ 210^(11) L_⊙, for H_0 = 75 km s^(-1) Mpc^(-1), have been observed in the H i line at Nançay and four of them were observed at Arecibo as well. Of these 19, ten had not been observed before. Six were clearly detected, one of which for the first time. The objective was to statistically sample the H i gas mass in luminous infrared mergers along a starburst merger sequence where the molecular CO gas content is already known. We also searched the literature for H i data and compared these with our observations.

Additional Information

© 2001 ESO. Received: 21 September 2000. Accepted: 22 December 2000. We would like to thank Drs. K. O'Neil and T. Ghosh for their help with the Arecibo observations and data reduction and Ms. M. Gendre for her help with the Nançay data reduction. We have made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the U.S. National Aeronautics and Space Administration, as well as the Lyon-Meudon Extragalactic Database (LEDA) supplied by the LEDA team at the CRAL-Observatoire de Lyon (France). The Unité Scientifique Nançay of the Observatoire de Paris is associated as Unité de Service et de Recherche USR No. B704 to the French Centre National de Recherche Scientifique (CNRS). Nançay also gratefully acknowledges the financial support of the Département du Cher, the European Community, the FNADT and the Région Centre.

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Submitted - 0101003.pdf

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Additional details

Created:
August 19, 2023
Modified:
October 18, 2023