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The B[e] phenomenon in the Milky Way and Magellanic Clouds

Published online by Cambridge University Press:  12 July 2011

Anatoly S. Miroshnichenko ,
Nadine Manset ,
Francesco Polcaro ,
Corinne Rossi  and
Sergey Zharikov
Anatoly S. Miroshnichenko
Affiliation:
Dept. of Physics & Astronomy, University of North Carolina at Greensboro, P.O. Box 26170, Greensboro, NC 27402–6170, USA email: a_mirosh@uncg.edu
Nadine Manset
Affiliation:
CFHT Corporation, 65–1238 Mamalahoa Highway, Kamuela, HI 96743
Francesco Polcaro
Affiliation:
Istituto di Astrofisica Spaziale e Fisica Cosmica, INAF, Via del Fosso del Cavaliere 100, 00133, Roma, Italy
Corinne Rossi
Affiliation:
Universitá La Sapienza Roma - Pza A Moro 5, I–00162 Roma, Italy
Sergey Zharikov
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, Apartado Postal 877, 22800, Ensenada, BC, Mexico
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Abstract

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Discovered over 30 years ago, the B[e] phenomenon has not yet revealed all its puzzles. New objects that exhibit it are being discovered in the Milky Way, and properties of known objects are being constrained. We review recent findings about objects of this class and their subgroups as well as discuss new results from studies of the objects with yet unknown nature. In the Magellanic Clouds, the population of such objects has been restricted to supergiants. We present new candidates with apparently lower luminosities found in the LMC.

Keywords

stars: early-typeinfrared: starscircumstellar matter
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S272: Active OB stars: structure, evolution, mass loss, and critical limits , July 2010 , pp. 260 - 264
Copyright
Copyright © International Astronomical Union 2011

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