Call for a photometric campaign on HR 8851
Abstract
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.
- Publication:
-
Delta Scuti Star Newsletter
- Pub Date:
- March 1994
- Bibcode:
- 1994DSSN....7...18J