A dust shell around the yellow supergiant CoD -61 deg 3326

Details A dust shell around the yellow supergiant CoD -61 deg 3326 A dust shell around the yellow supergiant CoD -61 deg 3326

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pasp...94..669t&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 94, Aug. 1982, p. 669-671.

Astronomy and Astrophysics

Astronomy

8

Cosmic Dust, Stellar Envelopes, Stellar Spectrophotometry, Supergiant Stars, Broadband, F Stars, Infrared Astronomy, Spectral Energy Distribution

Scientific paper

Broad-band photometry from 1-4 microns and low-resolution spectrometry, in the 2-micron atmospheric window, of the F-type supergiant CoD -61 deg 3326 equals Hz 747 are reported. The presence of an optically thin dust shell around this star is deduced and its properties are discussed with reference to the well-known yellow supergiant 89 Her. A similar post-main-sequence evolutionary status is proposed for both stars.

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