Near-infrared observations of the peculiar binary system epsilon Aurigae

Details Near-infrared observations of the peculiar binary system epsilon Aurigae Near-infrared observations of the peculiar binary system epsilon Aurigae

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.104..293b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 104, no. 2, Sept. 1984, p. 293-296.

Astronomy and Astrophysics

Astronomy

1

Eclipsing Binary Stars, Infrared Astronomy, Peculiar Stars, Stellar Spectrophotometry, Black Body Radiation, Near Infrared Radiation, Stellar Temperature, Wavelengths

Scientific paper

Near-infrared photometric and low-resolution spectroscopic observations of epsilon Aurigae at two phases during the current eclipse are presented. The eclipse depths are found to be wavelength-independent in the infrared right up to 2.5 microns. There is no infrared excess at wavelengths shorter than 2.5 microns. The light absorbing particles in the eclipsing body must be larger than 10 microns in size.

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