IRAS observations of R Cor Bor stars

Details IRAS observations of R Cor Bor stars IRAS observations of R Cor Bor stars

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mnras.222..357k&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 222, Sept. 15, 1986, p. 357-364.

Astronomy and Astrophysics

Astronomy

30

Infrared Astronomy Satellite, Spaceborne Astronomy, Stellar Evolution, Stellar Spectrophotometry, Stellar Temperature, Variable Stars, Cosmic Dust, Red Giant Stars, Stellar Envelopes

Scientific paper

The IRAS observations of R Cr B, SU Tau and V 348 Sgr indicate the existence of a cool dust component of temperature about 30 K in R Cr B and SU Tau and less than or equal to 100 K in V 348 Sgr, in addition to the hot dust. It is suggested that this cool dust shell is a remnant of the stage when these stars were red giants for the first time. Although R Cr B was observed by IRAS during a visual light minimum no significant IR flux increase was apparent.

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