Light Variations of the B Star HR 7556

Details Light Variations of the B Star HR 7556 Light Variations of the B Star HR 7556

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.232..195b&link_type=abstract

Astrophysics and Space Science, Volume 232, Issue 1, pp.195-199

Astronomy and Astrophysics

Astrophysics

Scientific paper

On the basis of newU BV photometry this paper reports on the discovery
of the variability of the B star HR 7556. The ellipsoidal character of
the light curve indicates that it is probably a long period (P ˜
40d) interacting binary. This interpretation has been
confirmed by available radial velocity data.

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