Reference : Studying bright, massive stars in the era of large telescopes I. General context

	Document type :	Scientific journals : Article
	Discipline(s) :	Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
	To cite this reference:	http://hdl.handle.net/2268/73899

Title :	Studying bright, massive stars in the era of large telescopes I. General context
Language :	English
Author, co-author :	Rauw, Grégor [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Sciences spatiales >]
Publication date :	1-Jun-2010
Journal title :	Bulletin de la Société Royale des Sciences de Liège
Volume :	79
Pages :	25
Audience :	International
ISSN :	0037-9565
Keywords :	[en] stars: massive ; stars: fundamental parameters ; stars: emission-line ; stars: winds ; outflows ; stars: binaries: general
Abstract :	[en] Stars of spectral type O play a key role in many processes in our Galaxy and beyond. However, there are still a number of open issues about these massive and luminous objects that need to be ad-dressed. Several of these questions require (long-term) spectroscopic monitoring that is difficult to achieve with the highly-demanded equipment on most modern professional instruments. However, these kinds of studies offer an opportunity for collaborations between amateur spectroscopists and professional astrophysicists.
Permalink :	http://hdl.handle.net/2268/73899
Other URL :	http://adsabs.harvard.edu/abs/2010BSRSL..79...25R

	File(s) associated to this reference
	Fulltext file(s): File Commentary Version Size Access Restricted access Rauw Vol79 2010 p 25-37.pdf No commentary Publisher postprint 688.3 kB Request copy

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