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dc.contributor.authorGünther, H.M.
dc.contributor.authorWolk, S.J.
dc.contributor.authorSpitzbart, B.
dc.contributor.authorForbrich, J.
dc.contributor.authorWright, N.J.
dc.contributor.authorBourke, T.L.
dc.contributor.authorGutermuth, R.A.
dc.contributor.authorAllen, L.
dc.contributor.authorMegeath, S.T.
dc.contributor.authorPipher, J.L.
dc.date.accessioned2013-02-06T10:00:09Z
dc.date.available2013-02-06T10:00:09Z
dc.date.issued2012-10-01
dc.identifier.citationGünther , H M , Wolk , S J , Spitzbart , B , Forbrich , J , Wright , N J , Bourke , T L , Gutermuth , R A , Allen , L , Megeath , S T & Pipher , J L 2012 , ' IRAS 20050+2720 : Anatomy of a young stellar cluster ' , The Astronomical Journal , vol. 144 , no. 4 , 101 . https://doi.org/10.1088/0004-6256/144/4/101
dc.identifier.issn0004-6256
dc.identifier.otherPURE: 1268547
dc.identifier.otherPURE UUID: f1e91c49-8067-4716-872e-0008c52288da
dc.identifier.otherScopus: 84866384230
dc.identifier.urihttp://hdl.handle.net/2299/9912
dc.descriptionCopyright 2012 Elsevier B.V., All rights reserved.
dc.description.abstractIRAS 20050+2720 is young star-forming region at a distance of 700 pc without apparent high-mass stars. We present results of our multi-wavelength study of IRAS 20050+2720 which includes observations by Chandra and Spitzer, and Two Micron All Sky Survey and UBVRI photometry. In total, about 300 young stellar objects (YSOs) in different evolutionary stages are found. We characterize the distribution of YSOs in this region using a minimum spanning tree analysis. We newly identify a second cluster core, which consists mostly of class II objects, about 10' from the center of the cloud. YSOs of earlier evolutionary stages are more clustered than more evolved objects. The X-ray luminosity function (XLF) of IRAS 20050+2720 is roughly lognormal, but steeper than the XLF of the more massive Orion Nebula complex. IRAS 20050+2720 shows a lower N H/AK ratio compared with the diffuse interstellar mediumen
dc.language.isoeng
dc.relation.ispartofThe Astronomical Journal
dc.titleIRAS 20050+2720 : Anatomy of a young stellar clusteren
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=84866384230&partnerID=8YFLogxK
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1088/0004-6256/144/4/101
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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