R Coronae Borealis in 1988

Details R Coronae Borealis in 1988 R Coronae Borealis in 1988

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pasp..102..162f&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 102, Feb. 1990, p. 162-165.

Astronomy and Astrophysics

Astronomy

13

Supergiant Stars, Ubv Spectra, Variable Stars, Fourier Transformation, Stellar Color, Stellar Spectrophotometry

Scientific paper

UBV photometry of R CrB on 99 nights during 1988 is presented. The star
was close to maximum light during these 5 months and showed its usual
small variability of about 0.2 mag in V. However, a period analysis
reveals no sign of the customary 44-day period; instead, periods of
about 59, 31, and possibly 23 days were present.

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