Photometry of \varepsilon Aurigae in the Near-Infrared Range Before the Next Expected Primary Eclipse

Details Photometry of \varepsilon Aurigae in the Near-Infrared Range Before the Next Expected Primary Eclipse Photometry of \varepsilon Aurigae in the Near-Infrared Range Before the Next Expected Primary Eclipse

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010vsgh.conf..210m&link_type=abstract

Variable Stars, the Galactic halo and Galaxy Formation, Proceedings of an international conference held in Zvenigorod, Russia, 1

Astronomy and Astrophysics

Astronomy

Scientific paper

The results of photometric measurements of the eclipsing variable \varepsilon Aur obtained in 1980-2009 in the 1-5 μm spectral range are presented. Observations in the 3.5-5 μm range exhibit an excess relative to the light from the F supergiant, which corresponds to emission from a cool source with temperature ˜ 400-1000 K. Neutral character of absorption was observed during the eclipse.

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