Hαemission line spectroscopy in NGC 330-Reference-Cited by-同舟云学术

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Hαemission line spectroscopy in NGC 330

Published:2001-06 Issue:3 Volume:371 Page:932-942
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Hummel W.,Gässler W.,Muschielok B.,Schink H.,Nicklas H.,Conti G.,Mattaini E.,Keller S.,Mantel K.-H.,Appenzeller I.,Rupprecht G.,Seifert W.,Stahl O.,Tarantik K.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20010386/pdf

Reference53 articles.

1. Böhnhardt, H. (ed.) 2000, FORS1+2 User Manual, VLT-MAN-ESO-13100-1543/1.5

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1. The XMM-Newton survey of the Small Magellanic Cloud: XMMU J010633.1−731543 and XMMU J010743.1−715953, two new Be/X-ray binary systems★;Monthly Notices of the Royal Astronomical Society;2012-06-15

2. A slitless spectroscopic survey for Hαemission-line objects in SMC clusters;Astronomy and Astrophysics;2010-01

3. Be stars and binaries in the field of the SMC open cluster NGC 330 with VLT-FLAMES;Astronomy & Astrophysics;2007-07-16

4. The VLT-FLAMES survey of massive stars: observations centered on the Magellanic Cloud clusters NGC 330, NGC 346, NGC 2004, and the N11 region;Astronomy & Astrophysics;2006-08-31

5. A Be star with a low nitrogen abundance in the SMC cluster NGC 330;Astronomy & Astrophysics;2005-07

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