The variability of HR 8062

Details The variability of HR 8062 The variability of HR 8062

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pasp..103..559f&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 103, June 1991, p. 559, 560.

Astronomy and Astrophysics

Astronomy

1

S Stars, Technetium, Variable Stars, Fourier Transformation, Least Squares Method, Light Curve, Stellar Oscillations

Scientific paper

HR 8062, the only S star known to show technetium while not being a
large-amplitude photometric variable, has been checked for variability.
Snyder's 1990 discovery that it is a low-amplitude variable is confirmed
and a single period of 34.3 days derived.

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