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Article: Mapping the outflow from G5.89-0.39 in SiO J = 5 → 4

TitleMapping the outflow from G5.89-0.39 in SiO J = 5 → 4
Authors
KeywordsH Ii Regions
Ism: Individual (G5.89-0.39)
Ism: Jets And Outflows
Stars: Formation
Issue Date2004
PublisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205
Citation
Astrophysical Journal Letters, 2004, v. 616 n. 1 II, p. L35-L38 How to Cite?
AbstractWe have mapped the ultracompact H II region, G5.89-0.39, and its molecular surroundings with the Sub-millimeter Array at 2″.8 × 1″.8 angular resolution in 1.3 mm continuum, SiO J = 5 → 4, and eight other molecular lines. We have resolved for the first time the highly energetic molecular outflow in this region. At this resolution, the outflow is definitely bipolar and appears to originate in a 1.3 mm continuum source. The continuum source peaks in the center of the H II region. The axis of the outflow lines up with a recently discovered O5 V star.
Persistent Identifierhttp://hdl.handle.net/10722/174927
ISSN
2015 Impact Factor: 5.487
2015 SCImago Journal Rankings: 3.369
References

 

DC FieldValueLanguage
dc.contributor.authorSollins, PKen_US
dc.contributor.authorHunter, TRen_US
dc.contributor.authorBattat, Jen_US
dc.contributor.authorBeuther, Hen_US
dc.contributor.authorHo, PTPen_US
dc.contributor.authorLim, Jen_US
dc.contributor.authorLiu, SYen_US
dc.contributor.authorOhashi, Nen_US
dc.contributor.authorSridharan, TKen_US
dc.contributor.authorSu, YNen_US
dc.contributor.authorZhao, JHen_US
dc.contributor.authorZhang, Qen_US
dc.date.accessioned2012-11-26T08:48:12Z-
dc.date.available2012-11-26T08:48:12Z-
dc.date.issued2004en_US
dc.identifier.citationAstrophysical Journal Letters, 2004, v. 616 n. 1 II, p. L35-L38en_US
dc.identifier.issn2041-8205en_US
dc.identifier.urihttp://hdl.handle.net/10722/174927-
dc.description.abstractWe have mapped the ultracompact H II region, G5.89-0.39, and its molecular surroundings with the Sub-millimeter Array at 2″.8 × 1″.8 angular resolution in 1.3 mm continuum, SiO J = 5 → 4, and eight other molecular lines. We have resolved for the first time the highly energetic molecular outflow in this region. At this resolution, the outflow is definitely bipolar and appears to originate in a 1.3 mm continuum source. The continuum source peaks in the center of the H II region. The axis of the outflow lines up with a recently discovered O5 V star.en_US
dc.languageengen_US
dc.publisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205en_US
dc.relation.ispartofAstrophysical Journal Lettersen_US
dc.subjectH Ii Regionsen_US
dc.subjectIsm: Individual (G5.89-0.39)en_US
dc.subjectIsm: Jets And Outflowsen_US
dc.subjectStars: Formationen_US
dc.titleMapping the outflow from G5.89-0.39 in SiO J = 5 → 4en_US
dc.typeArticleen_US
dc.identifier.emailLim, J: jjlim@hku.hken_US
dc.identifier.authorityLim, J=rp00745en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.scopuseid_2-s2.0-12344314065en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-12344314065&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume616en_US
dc.identifier.issue1 IIen_US
dc.identifier.spageL35en_US
dc.identifier.epageL38en_US
dc.publisher.placeUnited Kingdomen_US
dc.identifier.scopusauthoridSollins, PK=7004013438en_US
dc.identifier.scopusauthoridHunter, TR=35394114700en_US
dc.identifier.scopusauthoridBattat, J=55318519400en_US
dc.identifier.scopusauthoridBeuther, H=10140586700en_US
dc.identifier.scopusauthoridHo, PTP=7402211489en_US
dc.identifier.scopusauthoridLim, J=7403453870en_US
dc.identifier.scopusauthoridLiu, SY=7409459358en_US
dc.identifier.scopusauthoridOhashi, N=7202558313en_US
dc.identifier.scopusauthoridSridharan, TK=6701592129en_US
dc.identifier.scopusauthoridSu, YN=35753955800en_US
dc.identifier.scopusauthoridZhao, JH=7410310692en_US
dc.identifier.scopusauthoridZhang, Q=8602636100en_US

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