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Spectroscopic surveys of faint blue starsSpectroscopy of 450 faint blue stars obtained with the spectrograph and intensified Reticon scanner on the 1.3 m telescope at the McGraw Hill Observatory located at Kitt Peak are examined. The study is limited to objects brighter than V = 17.0 in magnitude. It is found that the relative numbers of objects such as white dwarfs, QSOs and CVs in the Kisco survey (Noguchi et al. 1980) is similar to that in the survey of Green et al., (1986).
Document ID
19890030197
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Wegner, Gary
(Dartmouth Coll. Hanover, NH, United States)
Boley, Forrest I.
(Dartmouth Coll. Hanover, NH, United States)
Swanson, Steven R.
(Dartmouth College Hanover, NH, United States)
Mcmahan, Robert K.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1987
Subject Category
Astronomy
Meeting Information
Meeting: Conference on Faint Blue Stars
Location: Tucson, AZ
Country: United States
Start Date: June 1, 1987
End Date: June 5, 1987
Sponsors: IAU, NSF
Accession Number
89A17568
Funding Number(s)
CONTRACT_GRANT: NAG5-287
CONTRACT_GRANT: NSF AST-85-15219
Distribution Limits
Public
Copyright
Other

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