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The Strongly Polarized P Cygni Star with Infrared Excess CPD −52° 9243

Published online by Cambridge University Press:  14 August 2015

J. P. Swings
J. P. Swings*
Affiliation:
European Southern Observatory and Institut d'Astrophysique, Université de Liège

Abstract

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The visible spectrum of the point-like source with infrared excess CPD-52°9243 is identified; emission and absorption line strengths are given together with various ion velocities of P Cygni profiles; a strong polarization is detected: P ≃ 5 %, θ ≃ 36°. From stellar and interstellar features, a spectral type around B8Ia and a distance of about 3.1 kpcs are derived.

A detailed publication is presently in press in Astronomy and Astrophysics.

Type
II. Polarization
Information
Symposium - International Astronomical Union , Volume 98: Be Stars , 1982 , pp. 101 - 102
Copyright
Copyright © Reidel 1982