Spectrophotometric observations of UX ARIETIS

Details Spectrophotometric observations of UX ARIETIS Spectrophotometric observations of UX ARIETIS

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.183...11j&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 183, no. 1, Sept. 1991, p. 11-15.

Astronomy and Astrophysics

Astrophysics

Binary Stars, G Stars, K Stars, Stellar Atmospheres, Stellar Spectrophotometry, Spectral Energy Distribution, Stellar Models, Stellar Spectra, Stellar Temperature

Scientific paper

Spectrophotometric observations of the RS CVn binary UX Arietis are
presented. The comparison of the observed fluxes with model atmospheres
indicates that during the four phases observed, the temperature does not
vary significantly. However, brightness variation of 0.23 m are thought
to be due to change in the surface emitting regions.

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