Young stars and clouds in Camelopardalis

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dc.creatorStraizys, V.
dc.creatorLaugalys, V.
dc.date2008-11-18
dc.date.accessioned2026-07-07T10:19:13Z
dc.date.available2026-07-07T10:19:13Z
dc.descriptionStar formation in the Local spiral arm in the direction of the Galactic longitudes 132--158 deg is reviewed. Recent star-forming activity in this Milky Way direction is evidenced by the presence here of the Cam OB1 association and dense dust and molecular clouds containing H$α$ emission stars, young irregular variables and infrared stellar objects. The clouds of the Local arm concentrate in two layers at 150-300 pc and at about 900 pc from the Sun. The Perseus arm objects in this direction are at a distance of about 2 kpc.
dc.description14 pages, 6 figures
dc.identifierhttps://arxiv.org/abs/0811.2992
dc.identifierhttp://arxiv.org/abs/0811.2992
dc.identifierHandbook of Star Forming Regions, vol. 1, 2008, ASP
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/174428
dc.subjectAstrophysics
dc.titleYoung stars and clouds in Camelopardalis
dc.typetext

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