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Digicon photometry of an intergalactic bridgeSurface brightness and color data are derived for two points in the bridge and tail structure of Arp 295. The best observed point has a surface brightness in V of 25.9 magnitudes per square arc second and (B-V) = +1.00 m. A point on the tail is brighter with the same color.
Document ID
19750032211
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/129656
Authors
Beaver, E. A.
Harms, R. J. (California, University San Diego, Calif., United States)
Tifft, W. G.
Sargent, T. A. (Steward Observatory Tucson, Ariz., United States)
Date Acquired
August 8, 2013
Publication Date
October 1, 1974
Publication Information
Publication: Astronomical Society of the Pacific
Subject Category
Astronomy
Accession Number
75A16283
Funding Number(s)
CONTRACT_GRANT: NGR-05-009-188
CONTRACT_GRANT: NGL-05-005-007
Distribution Limits
Public
Copyright
Other

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