Photoelectric monitoring of a shell star in Perseus

Details Photoelectric monitoring of a shell star in Perseus Photoelectric monitoring of a shell star in Perseus

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984acasn..25..136c&link_type=abstract

(Acta Astronomica Sinica, vol. 25, no. 2, 1984, p. 136-141) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 8, Dec. 19

Astronomy and Astrophysics

Astrophysics

Astronomical Photometry, B Stars, Electrophotometry, Shell Stars, Nebulae, Stellar Color

Scientific paper

Three-color photoelectric monitoring of the shell star in Perseus, discovered by Chu (1978), is reported. On the night of Feb. 4-5, 1983, this star still showed obvious light variations, although the amplitude was less than in 1979. On the next night, the light variation was close to the observing error. It is inferred that the shell activity is now at a stable phase for a few years.

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