The infrared spectrum of the peculiar star HDE 316285

Details The infrared spectrum of the peculiar star HDE 316285 The infrared spectrum of the peculiar star HDE 316285

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983obs...103..255w&link_type=abstract

The Observatory, vol. 103, p. 255-257 (1983)

Physics

2

Scientific paper

The P-Cygni star HDE 316285 is probably a heavily reddened single star
undergoing mass-loss, rather than a symbiotic system. The infrared
continuum is from the Rayleigh-Jeans tail of a high-temperature source
plus emission from a hot plasma. The 1.2 - 4.1-μm spectrum shows
strong emission lines, mainly of H I and He I.

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