H alpha emission from pre-main sequence stars

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Show simple item record Fernandez, M Ortiz, E Eiroa, C Miranda, LF 2011-01-22T10:28:26Z 2011-01-22T10:28:26Z 1995
dc.identifier.issn 0365-0138
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

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