Detection of optical variability of LSI + 61 deg 303

Details Detection of optical variability of LSI + 61 deg 303 Detection of optical variability of LSI + 61 deg 303

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...154l..30p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 154, no. 1-2, Jan. 1986, p. L30-L32.

Astronomy and Astrophysics

Astrophysics

30

Early Stars, Periodic Variations, Radio Stars, Stellar Spectrophotometry, Visible Spectrum, X Ray Binaries, Spectrum Analysis, Stellar Color, Stellar Luminosity, Stellar Magnitude, Ubv Spectra

Scientific paper

The authors report the detection of optical variability of the star LSI+61°303 obtained from UBVRI photometric observations. The optical light varies by about 0.1 magnitude over a 10-day time interval. An analysis of the spectral type and luminosity class of the star is presented and discussed. Some results of radio observations are also presented.

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