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

被引：8
|
作者：
Miroshnichenko, Anatoly S. [1 ]
Manset, Nadine [2 ]
Polcaro, Francesco [3 ]
Rossi, Corinne [4 ]
Zharikov, Sergey [5 ]
机构：
[1] Univ N Carolina, Dept Phys & Astron, POB 26170, Greensboro, NC 27402 USA
[2] CFHT Corp, Kamuela, HI 96743 USA
[3] INAF, Ist Astrofis Spaziale & Fis Cosm, I-00133 Rome, Italy
[4] Univ Roma La Sapienza, I-00162 Rome, Italy
[5] Univ Nacl Autonoma Mexico, Inst Astron, Ensenada 22800, Baja California, Mexico
来源：
ACTIVE OB STARS: STRUCTURE, EVOLUTION, MASS-LOSS, AND CRITICAL LIMITS | 2011年 / 272期
基金：
美国国家航空航天局; 美国国家科学基金会;
关键词：
stars: early-type; infrared: stars; circumstellar matter; GALACTIC FSCMA STARS; SUPERGIANTS; CATALOG;
D O I：
10.1017/S1743921311010507
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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.
引用
收藏
页码：260 / +
页数：3
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