WHT observations of cataclysmic variables in globular clusters. I - V101 in M5 during quiescence and outburst

Details WHT observations of cataclysmic variables in globular clusters. I - V101 in M5 during quiescence and outburst WHT observations of cataclysmic variables in globular clusters. I - V101 in M5 during quiescence and outburst

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.241p..25n&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 241, Nov. 1, 1989, p. 25P-30P.

Astronomy and Astrophysics

Astronomy

17

Cataclysmic Variables, Globular Clusters, Stellar Spectrophotometry, Dwarf Novae, Light Curve, Radial Velocity, Stellar Color, Stellar Magnitude

Scientific paper

WHT spectroscopy and photometry are used to investigate the structure of the cataclysmic vaiable V101, in the globular cluster M5. An encouraging consistency is found between the properties derived from the color, magnitude, radial-velocity variations and outburst light curve. All these indicate that V101's orbital period lies above the period gap, is at the distance of M5, and is probably a dwarf nova.

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