Hamuy's blue variable star in Orion

Details Hamuy's blue variable star in Orion Hamuy's blue variable star in Orion

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pasp...99.1097b&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 99, Oct. 1987, p. 1097, 1098.

Astronomy and Astrophysics

Astronomy

10

Blue Stars, Cataclysmic Variables, Dwarf Novae, Orion Constellation, Stellar Spectra, Astronomical Photometry, High Speed Photography, Light Curve

Scientific paper

High-speed photometry of Hamuy's (Hamuy and Maza, 1986) blue variable star in Orion, obtained on September 26 and 28, 1986 with the two-star photometer of the University of Arkansas at Little Rock attached to the 1.3-m Kitt Peak National Observatory reflector, are presented. Both the short-time-scale flickering and the spectroscopic appearance of the star are found to be typical of the class of nova-like (UX UMa-type) variables. The data suggest that Hamuy's variable does not range over more than a few tenths of a magnitude.

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