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)