SPECTROSCOPIC MONITORING OF THE B[E] OBJECTS FSCMA AND MOCAM

Objects with the B[e] phenomenon exhibit permitted and forbidden emission lines due to the presence of circumstellar ionized gas and large infrared excesses due to processing of the stellar radiation by circumstellar dust. There are five groups of stars that show this phenomenon (pre-main-sequence H...

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Bibliographic Details
Main Authors: A. K. Kuratova, A. S. Miroshnichenko, S. V. Zharikov, N. Manset, S. A. Khokhlov, A. Raj, A. V. Kusakin, I. V. Reva, R. I. Kokumbaeva, I. A. Usenko, A. Y. Knyazev
Format: Article
Language:English
Published: Odessa I. I. Mechnykov National University 2019-10-01
Series:Odessa Astronomical Publications
Online Access:http://oap.onu.edu.ua/article/view/182100