H alpha emission from pre-main sequence stars

dc.contributor.author	Fernandez, M
dc.contributor.author	Ortiz, E
dc.contributor.author	Eiroa, C
dc.contributor.author	Miranda, LF
dc.date.accessioned	2011-01-22T10:28:26Z
dc.date.available	2011-01-22T10:28:26Z
dc.date.issued	1995
dc.identifier.issn	0365-0138
dc.identifier.uri	http://hdl.handle.net/11154/3413
dc.description.abstract	We present the results of an Her emission line observational study of a sample of 75 pre-main sequence stars consisting of 17 HAEBE, 47 CTT and 11 WTT stars. Approximately half of the stars are faint, with a brightness in the V band greater than or similar to 13. The spectra have been taken at resolutions approximate to 30 km s(-1) and approximate to 80 km s(-1). The data shown provide information on equivalent width, radial velocity, variability and line profile.	en_US
dc.language.iso	en	en_US
dc.title	H alpha emission from pre-main sequence stars	en_US
dc.type	Article	en_US
dc.identifier.idprometeo	3133
dc.source.novolpages	114(3):439-464
dc.subject.wos	Astronomy & Astrophysics
dc.description.index	WoS: SCI, SSCI o AHCI
dc.subject.keywords	stars, formation
dc.subject.keywords	stars, pre-main sequence
dc.subject.keywords	line, profiles
dc.relation.journal	Astronomy & Astrophysics Supplement Series