WHT observations of cataclysmic variables in globular clusters. II - The CV candidates in M71

Details WHT observations of cataclysmic variables in globular clusters. II - The CV candidates in M71 WHT observations of cataclysmic variables in globular clusters. II - The CV candidates in M71

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.242p...9m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 242, Jan. 1, 1990, p. 9P-13P.

Astronomy and Astrophysics

Astronomy

1

Cataclysmic Variables, Globular Clusters, Stellar Spectrophotometry, Ultraviolet Astronomy, Balmer Series, Subdwarf Stars, White Dwarf Stars

Scientific paper

Results are presented from photometric and spectroscopic observations of the six UV-bright objects in M71 which Richer and Fahlman (1988) proposed as candidate cataclysmic variables. It is found that the two brightest of these candidates are probably hot subdwarfs. It is suggested that the remaining candidates are more likely to be white dwarfs and subdwarfs than cataclysmic variables.

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