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Resolved CO(1-0) Nuclei in IRAS 14348-1447: Evidence for Massive Bulge Progenitors to Ultraluminous Infrared GalaxiesThe CO morphology shows two molecular gas components associated with the stellar nuclei of the progenitors, consistent with the idea that the molecular disks are gravitationally bound by the dense bulges of the progenitor galaxies as the interaction proceeds.
Document ID
20060034576
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
hdl:2014/18891
Authors
Surace, J.
Evans, A.
Mazzarella, J.
Date Acquired
August 23, 2013
Publication Date
November 1, 1999
Publication Information
Publication: Astrophysical Journal Letters
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Other
Keywords
nuclei galaxies IRAS 14348-1447

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