An infrared candidate for OH 205.1-14.1

Details An infrared candidate for OH 205.1-14.1 An infrared candidate for OH 205.1-14.1

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.192..805a&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 192, Sept. 1980, p. 805-807.

Astronomy and Astrophysics

Astronomy

10

Dwarf Stars, Hydroxyl Emission, Infrared Astronomy, Late Stars, Radiation Sources, Stellar Spectrophotometry, B Stars, Interplanetary Dust, Stellar Envelopes, Stellar Evolution, Water

Scientific paper

An infrared source coincident with the OH and H2O complex OH 205.1-14.1
in the Lynds 1630 dark cloud has been located. The infrared source is
probably a late B dwarf embedded in a circumstellar dust cloud.

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