The B[e] phenomenon in the Milky Way and Magellanic Clouds
Anatoly Miroshnichenko (University of North Carolina at Greensboro,, NC, USA), Nadine Manset (CFHT Corporation, Kamuela, HI, USA), Francesco, Polcaro (Istituto di Astrofisica Spaziale e Fisica Cosmica, INAF, Roma,, Italy) Corinne Rossi (Universit\'a La Sapienza Roma, Italy)
TL;DR
This paper reviews recent discoveries and studies of the B[e] phenomenon in the Milky Way and Magellanic Clouds, highlighting new candidates and the ongoing effort to understand this complex stellar behavior.
Contribution
It provides an updated overview of B[e] objects, including newly identified candidates and insights into their properties and classifications in different galactic environments.
Findings
New B[e] candidates identified in the LMC
Properties of known B[e] objects are being better constrained
The population of B[e] supergiants in the Magellanic Clouds is expanding
Abstract
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.
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