Photometric variability for the VV Cephei-like star HR 8164

Details Photometric variability for the VV Cephei-like star HR 8164 Photometric variability for the VV Cephei-like star HR 8164

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pasp..103..310h&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 103, March 1991, p. 310-312.

Astronomy and Astrophysics

Astronomy

Astronomical Photometry, Eclipsing Binary Stars, Irregular Variable Stars, M Stars, Supergiant Stars, Emission Spectra, Forbidden Transitions, H Alpha Line, Stellar Spectra

Scientific paper

HR 8164, a VV Cephei-like star, has been found to be photometrically
variable over a range of about 0.2 V magnitude and a cycle time of
several years. This variation is likely of an irregular type and does
not seem to be accompanied by a color change.

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