The Lacerta OB1 Association

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dc.creatorChen, W. P.
dc.creatorLee, H. T.
dc.date2008-11-04
dc.date.accessioned2026-07-07T10:15:21Z
dc.date.available2026-07-07T10:15:21Z
dc.descriptionLac OB1 is a nearby OB association in its final stage of star formation. While the member stars suggest an expansion time scale of tens of Myr, the latest star formation episode, as manifested by the existence of massive and pre-main sequence stars, took place no more than a few Myr ago. The remnant molecular clouds in the region provide evidence of starbirth triggered by massive stars.
dc.descriptionto appear in the Handbook of Star Forming Regions, Vol. I, edited by Bo Reipurth
dc.identifierhttps://arxiv.org/abs/0811.0443
dc.identifierhttp://arxiv.org/abs/0811.0443
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/173149
dc.subjectAstrophysics
dc.titleThe Lacerta OB1 Association
dc.typetext

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