Young Stars in the Camelopardalis Dust and Molecular Clouds. IV. Spectral Observations of the Suspected YSOs

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dc.creatorCorbally, C. J.
dc.creatorStraizys, V.
dc.date2008-09-13
dc.date.accessioned2026-07-07T10:02:46Z
dc.date.available2026-07-07T10:02:46Z
dc.descriptionIn the first three papers of this series, about 200 objects in Camelopardalis and the nearby areas of Cassiopeia, Perseus and Auriga were suspected of being pre-main-sequence stars in different stages of evolution. To confirm the evolutionary status of the 15 brightest objects, their far-red range (600--950 nm) spectra were obtained. Almost all these objects are young stars with emissions in H alpha, OI, CaII and P9 lines. The equivalent widths of emission lines and approximate spectral classes of the objects are determined.
dc.description17 pages
dc.identifierhttps://arxiv.org/abs/0809.2355
dc.identifierhttp://arxiv.org/abs/0809.2355
dc.identifierBaltic Astronomy, vol. 17, 21-37, 2008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/169090
dc.subjectAstrophysics
dc.titleYoung Stars in the Camelopardalis Dust and Molecular Clouds. IV. Spectral Observations of the Suspected YSOs
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