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The interacting galaxy pair NGC 4485 and NGC 4490 - Star formation and the interstellar mediumThe 100- and 160-micron continuum emission from cool dust in the interacting gas-rich pair of galaxies, NGC 4490 and NGC 4485, was mapped. Visual continuum and H-alpha images of the pair were obtained. The state of the interstellar medium and the rate and efficiency of star formation are investigated.
Document ID
19890049472
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/167337
Authors
Thronson, Harley A., Jr. (Wyoming Infrared Observatory Laramie, United States)
Hunter, Deidre A. (Lowell Observatory Flagstaff, AZ, United States)
Casey, Sean (Wyoming Univ. Laramie, WY, United States)
Harper, D. A. (Yerkes Observatory Williams Bay, WI, United States)
Latter, William B. (Steward Observatory Tucson, AZ, United States)
Date Acquired
August 14, 2013
Publication Date
April 15, 1989
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 339
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
89A36843
Funding Number(s)
CONTRACT_GRANT: NAG2-134
Distribution Limits
Public
Copyright
Other

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