WHT observations of cataclysmic variables in globular clusters. III - V4 in M30 during quiescence

Details WHT observations of cataclysmic variables in globular clusters. III - V4 in M30 during quiescence WHT observations of cataclysmic variables in globular clusters. III - V4 in M30 during quiescence

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.250..602m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 250, June 1, 1991, p. 602-606.

Astronomy and Astrophysics

Astronomy

6

Cataclysmic Variables, Dwarf Novae, Globular Clusters, Spectral Line Width, Stellar Color, Stellar Magnitude, Stellar Spectrophotometry, Telescopes

Scientific paper

The results of William Herschel telescope (WHT) obsevations of the candidate globular-cluster dwarf nova, V4 in M30 are reported. It is found that, on the basis of its quiescent magnitude and colors, its outburst magnitude and its radial velocity, V4 is likely to be a foreground object in the field of M30. In addition, it is probably a short-period system near the period gap.

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