On the period of HR 1362

Details On the period of HR 1362 On the period of HR 1362

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pasp..101..677d&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 101, July 1989, p. 677-680. Research supported by the S

Other

2

Light Curve, Stellar Rotation, Stellar Spectrophotometry, Ubv Spectra, Variable Stars, Angular Velocity, Electrophotometry, H Lines, K Lines, Stellar Magnitude

Scientific paper

Photoelectric UBV observations, made in 1981 and 1982, of the active star HR 1362, are presented. A period analysis reveals many (all greater than 100 days) probable periods because of the large gaps in the data. If the most probable period around 330 d is true and represents the rotation period, as it does in all other active stars, then HR 1362 would be an extreme case of slow rotation.

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