Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4443
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dc.contributor.authorChoudhury, R-
dc.contributor.authorBhatt, H. C-
dc.date.accessioned2009-04-08T10:44:22Z-
dc.date.available2009-04-08T10:44:22Z-
dc.date.issued2009-03-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Vol. 393, No. 3, pp. 959 - 968en
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/2248/4443-
dc.descriptionThe original publication is available aten
dc.description.abstractAn analysis of the proper motion measurements of the young stellar objects (YSOs) associated with the cometary globules (CGs) in the Gum Nebula is presented. While earlier studies based on the radial-velocity measurements of the CGs suggested expansion of the system of the CGs, the observed proper motion of the YSOs shows no evidence for expansion. In particular, the kinematics of two YSOs embedded in CGs are inconsistent with the supernova explosion of the companion of ζ Pup, about 1.5 Myr ago being the cause of the expansion of the system of the CGs. YSOs associated with the CGs share the average proper motion of the member stars of the Vela OB2 association. A few YSOs that have relatively large proper motions are found to show relatively low infrared excesses.en
dc.language.isoenen
dc.publisherRoyal Astronomical Societyen
dc.relation.urihttp://arxiv.org/abs/0811.4389en
dc.relation.urihttp://dx.doi.org/10.1111/j.1365-2966.2008.14189.xen
dc.rights© Royal Astronomical Societyen
dc.subjectStars: Pre-Main-Sequenceen
dc.subjectKinematicsen
dc.subjectISM: Globulesen
dc.subjectClouds and HII Regions: Individual: Gum Nebulaen
dc.titleKinematics of the young stellar objects associated with the cometary globules in the Gum Nebulaen
dc.typeArticleen
Appears in Collections:IIAP Publications



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