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Global properties of the nearby spiral M101M101 (NGC 5457) is a classic Sc I spiral galaxy located suffiently nearby, 6.8 Mpc, that its structure can be studied even with the coarse angular resolution of the Infrared Astronomy Satellite (IRAS). The global infrared properties of M101 are addressed including the radial dependence of its infrared emission.
Document ID
19870014876
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Beichman, C. (California Inst. of Tech. Pasadena, CA, United States)
Boulanger, F. (California Inst. of Tech. Pasadena, CA, United States)
Rice, W. (California Inst. of Tech. Pasadena, CA, United States)
Persson, Carol J. Lonsdale (California Inst. of Tech. Pasadena, CA, United States)
Viallefond, F. (Institut d'Astrophysique Paris, France)
Date Acquired
September 5, 2013
Publication Date
May 1, 1987
Publication Information
Publication: NASA, Washington Star Formation in Galaxies
Subject Category
Astrophysics
Accession Number
87N24309
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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