The large globule Lynds 810 as a possible member of the Vulpecula OB1 complex

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dc.creator Turner, David Gerald, 1945-
dc.date.accessioned 2016-11-21T18:18:09Z
dc.date.available 2016-11-21T18:18:09Z
dc.date.issued 1986-10
dc.identifier.issn 0004-6361
dc.identifier.uri http://library2.smu.ca/handle/01/26681
dc.description Publisher's version/PDF en_CA
dc.description.abstract A distance of 2.5 [plus or minus] 0.2 kpc is derived for the dark globule Lynds 810 using photometric data for foreground stars and star counts. It is argued that this globule is likely to belong to the Vul OB1 complex. Its cometary structure, like certain other features of dust-related objects in Vulpecula, appears to be the shock signature of a past disturbance originating from a region near l = 60[degrees symbol], b = +2[degrees symbol], which lies within the fossil H II region Lynds 792. en_CA
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dc.language.iso en en_CA
dc.publisher EDP Sciences en_CA
dc.relation.uri http://www.aanda.org/
dc.rights Article is made available in accordance with the publisher’s policy and is subject to copyright law. Please refer to the publisher’s site. Any re-use of this article is to be in accordance with the publisher’s copyright policy. This posting is in no way granting any permission for re-use to the reader/user.
dc.subject.lcsh Interstellar matter
dc.subject.lcsh Molecular clouds
dc.title The large globule Lynds 810 as a possible member of the Vulpecula OB1 complex en_CA
dc.type Text en_CA
dcterms.bibliographicCitation Astronomy and Astrophysics 167(1), 157-160. (1986) en_CA
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Article is made available in accordance with the publisher’s policy and is subject to copyright law. Please refer to the publisher’s site. Any re-use of this article is to be in accordance with the publisher’s copyright policy. This posting is in no way granting any permission for re-use to the reader/user.
 
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