HD96008 - Variable without a cause

Details HD96008 - Variable without a cause HD96008 - Variable without a cause

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...229..452m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 229, no. 2, March 1990, p. 452-456. Research supported by NSERC.

Astronomy and Astrophysics

Astrophysics

13

Binary Stars, Stellar Spectrophotometry, Ubv Spectra, Variable Stars, Early Stars, Infrared Photometry, Light Curve, Radial Velocity, Stellar Motions, Ultraviolet Photometry, Visual Photometry

Scientific paper

New photometry of HD96008 is reported which reveals that the star has an asymmetric light curve with a period near 0.31 d. Analysis of the data of Lampens (1987), combined with the new data, produces a period of 0.309873 + or - 0.000005 d. At present, there is no explanation for the variations of the star which can be reconciled with all the available data.

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