Molecules in celestial objects. II - IUE observations of CO towards Psi Persei /B5 Ve/

Details Molecules in celestial objects. II - IUE observations of CO towards Psi Persei /B5 Ve/ Molecules in celestial objects. II - IUE observations of CO towards Psi Persei /B5 Ve/

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.196...67t&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 196, July 1981, p. 67-71.

Astronomy and Astrophysics

Astronomy

2

Astronomical Spectroscopy, Carbon Monoxide, Hot Stars, Iue, Molecular Gases, Stellar Spectra, Absorption Spectra, B Stars, Shell Stars, Stellar Envelopes

Scientific paper

Absorption features corresponding to 1-0, 2-0, 3-0 and 4-0 bands of the
A-X transition of CO have been identified in the spectra of a hot shell
star, Psi Per (B5 Ve, E(B-V)=0.09). Arguments are put forward to suggest
its possible origin in the circumstellar shell.

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