Variable nature of PLEIONE

Details Variable nature of PLEIONE Variable nature of PLEIONE

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.174....1g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 174, no. 1, Dec. 1990, p. 1-11.

Astronomy and Astrophysics

Astrophysics

3

B Stars, Shell Stars, Variable Stars, Balmer Series, Emission Spectra, Light Curve, Stellar Envelopes, Stellar Spectrophotometry

Scientific paper

The long-term (from 1885 to 1986) behavior of Pleione was investigated by collecting data on its various parameters from different sources and displaying them simultaneously. It was found that different parameters show a long-term variability pattern and are well associated with each other during the course of variations. The analysis of the long-term behavior in the visible region showed that, since 1885, Pleione has passed through various phases: from Be to B, to the shell phase, to Be, to shell.

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