Photometry of the fast-rotating late-type star W92 in NGC 2264

Details Photometry of the fast-rotating late-type star W92 in NGC 2264 Photometry of the fast-rotating late-type star W92 in NGC 2264

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..89..395r&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 89, no. 2, Jan. 1983, p. 395-400.

Astronomy and Astrophysics

Astrophysics

1

Late Stars, Light Curve, Stellar Rotation, Stellar Spectrophotometry, Variable Stars, K Stars, Space Density

Scientific paper

The new light curve and the photometric UBVRI indices have been obtained. The star seems to be more densely and evenly covered by spots than before what results in a drop of mean brightness and in a longer duration of the minimum. The photometric indices still do not permit to estimate properly its luminosity: it can be a nearby K dwarf with some infrared excess or a reddened subgiant. Results of a fragmentary low-resolution spectroscopy are also reported.

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