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dc.contributor.authorMotogi, K.
dc.contributor.authorFujisawa, K.
dc.contributor.authorSugiyama, K.
dc.contributor.authorNiinuma, K.
dc.contributor.authorSorai, K.
dc.contributor.authorHonma, M.
dc.contributor.authorHirota, T.
dc.contributor.authorYonekura, Y.
dc.contributor.authorHachisuka, K.
dc.contributor.authorWalsh, Andrew
dc.contributor.editorUnknown
dc.date.accessioned2017-01-30T10:25:21Z
dc.date.available2017-01-30T10:25:21Z
dc.date.created2014-03-02T20:00:38Z
dc.date.issued2013
dc.identifier.citationMotogi, K. and Fujisawa, K. and Sugiyama, K. and Niinuma, K. and Sorai, K. and Honma, M. and Hirota, T. and Yonekura, Y. and Hachisuka, K. and Walsh, A.J. 2013. New Detection of an Extremely Blue-shift Dominated Jet in G353.273+0.641: A Possible Disk-Jet System on 100 AU Scale, in New Trends in Radio Astronomy in the ALMA Era: The 30th Anniversary of Nobeyama Radio Observatory, Dec 3-8 2012, pp. 381-381. Hakone, Japan: Astronomical Society of the Pacific.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/2706
dc.description.abstract

We report a new detection of an unusual molecular jet from a high mass protostellar object G353.273+0.641 using the NRO 45m telescope. Newly detected SiO (υ = 0, J = 2-1) jet shows highly blue-shift dominated spectrum similar to the associated 22 GHz maser emission. The remarkable blue-shift dominance in both of the maser and SiO emission can be caused by a compact (< 170 AU) and optically thick face-on disk, masking the red-shifted part of the jet.

dc.publisherAstronomical Society of the Pacific
dc.relation.urihttp://aspbooks.org/custom/publications/paper/476-0381.html
dc.titleNew Detection of an Extremely Blue-shift Dominated Jet in G353.273+0.641: A Possible Disk-Jet System on 100 AU Scale
dc.typeConference Paper
dcterms.source.startPage381
dcterms.source.endPage381
dcterms.source.titleNew Trends in Radio Astronomy in the ALMA Era: The 30th Anniversary of Nobeyama Radio Observatory
dcterms.source.seriesNew Trends in Radio Astronomy in the ALMA Era: The 30th Anniversary of Nobeyama Radio Observatory
dcterms.source.conferenceNew Trends in Radio Astronomy in the ALMA Era: The 30th Anniversary of Nobeyama Radio Observatory
dcterms.source.conference-start-dateAug 3 2012
dcterms.source.conferencelocationHakone, Japan
dcterms.source.placeSan Fransisco
curtin.department
curtin.accessStatusFulltext not available


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