A 2dF survey of the Small Magellanic Cloud

被引:128
作者
Evans, CJ
Howarth, ID
Irwin, MJ
Burnley, AW
Harries, TJ
机构
[1] Isaac Newton Grp Telescopes, Santa Cruz De La Palma 38700, Spain
[2] UCL, Dept Phys & Astron, London WC1E 6BT, England
[3] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
[4] Univ Exeter, Sch Phys, Exeter EX4 4QL, Devon, England
关键词
stars : early-type; stars; emission-line; Be; stars : fundamental parameters; Hertzsprung-Russell (HR) diagram; Magellanic Clouds;
D O I
10.1111/j.1365-2966.2004.08096.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a catalogue of new spectral types for hot, luminous stars in the Small Magellanic Cloud (SMC). The catalogue contains 4161 objects, giving an order-of-magnitude increase in the number of SMC stars with published spectroscopic classifications. The targets are primarily B- and A-type stars (2862 and 853 objects respectively), with one Wolf-Rayet, 139 O-type and 306 FG stars, sampling the main sequence to similar tomid-B. The selection and classification criteria are described, and objects of particular interest are discussed, including UV-selected targets from the Ultraviolet Imaging Telescope (UIT) experiment, Be and B[e] stars, 'anomalous A supergiants' and composite-spectrum systems. We examine the incidence of Balmer-line emission, and the relationship between Hgamma equivalent width and absolute magnitude for BA stars.
引用
收藏
页码:601 / 623
页数:23
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