Call for a photometric campaign on HR 8851

Details Call for a photometric campaign on HR 8851 Call for a photometric campaign on HR 8851

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994dssn....7...18j&link_type=abstract

Delta Scuti Star Newsletter, Issue 7, p. 18-21.

Physics

Scientific paper

HR 8851 was discovered by Hao and Huang (1993a) to be a variable star with a light period of 0.7 d and an amplitude of 0.21mag. This star is listed as F0IV type and spectroscopic binary in the Bright Star Catalogue (Hoffeit and Warren. 1991). According to its posilion in H-R diagram and its behaviour in light variation we amnounced that HR8851 is possibly a Delta Scuti star, though its variation period seems too long to fit such type stars.

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