dc.date.accessioned2019-12-18T18:14:58Z
dc.date.accessioned2022-10-18T22:34:38Z
dc.date.available2019-12-18T18:14:58Z
dc.date.available2022-10-18T22:34:38Z
dc.date.created2019-12-18T18:14:58Z
dc.date.issued2010
dc.identifierhttp://hdl.handle.net/10533/237197
dc.identifier15010003
dc.identifierWOS:000288431500007
dc.identifiereid=2-s2.0-78650414232
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4468535
dc.description.abstractIn this paper the southern cometary nebula GRV10 and its environment are investigated. The object is connected with a molecular cloud (its dimensions are ~4 pc). 12CO (1-0) observations toward GRV10 revealed the presence of two molecular outflows (a bipolar outflow), a red and a blue-shifted outflow, which coincide in position, indicating that they are moving along the line of sight in opposite directions. Near GRV10 a bright IR star, GRV10 IR, is discovered (near the southern edge of the nebula) and since its spectra and near IR colors favor it to be a Mira type star, a distance of ~4.4 kpc can be estimated. Star GRV10 IR appears connected with the IRAS point source IRAS 10406-6256. The grouping of stars (YSOs - young stellar objects) connected with GRV10 and embedded in a dark nebulosity is also discussed. This grouping is associated with the IRAS point source IRAS 10406-6253, which has FIR colors typical for embedded, not evolved, YSOs.
dc.languageeng
dc.relationhttps://link.springer.com/article/10.1007/s10511-010-9142-9
dc.relation10.1007/s10511-010-9142-9
dc.relationinfo:eu-repo/grantAgreement/Fondap/15010003
dc.relationinstname: Conicyt
dc.relationreponame: Repositorio Digital RI2.0
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.titleSouthern YSO GRV10 and its environment
dc.typeArticulo


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