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Article: Submillimeter Array multiline observations of the massive star-forming region IRAS 18089-1732

TitleSubmillimeter Array multiline observations of the massive star-forming region IRAS 18089-1732
Authors
KeywordsAstrochemistry
Line: Identification
Stars: Formation
Submillimeter
Techniques: Interferometric
Techniques: Spectroscopic
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. L19-L22 How to Cite?
AbstractSubmillimeter Array (SMA) observations of the high-mass star-forming region IRAS 18089-1732 in the 1 mm and 850 μm band with 1 GHz bandwidth reveal a wealth of information. We present the observations of 34 lines from 16 different molecular species. Most molecular line maps show significant contributions from the outflow, and only a few molecules are confined to the inner core. We present and discuss the molecular line observations and outline the unique capabilities of the SMA for future imaging line surveys at high spatial resolution.
Persistent Identifierhttp://hdl.handle.net/10722/174925
ISSN
2015 Impact Factor: 5.487
2015 SCImago Journal Rankings: 3.369
References

 

DC FieldValueLanguage
dc.contributor.authorBeuther, Hen_US
dc.contributor.authorZhang, Qen_US
dc.contributor.authorHunter, TRen_US
dc.contributor.authorSridharan, TKen_US
dc.contributor.authorZhao, JHen_US
dc.contributor.authorSollins, Pen_US
dc.contributor.authorHo, PTPen_US
dc.contributor.authorLiu, SYen_US
dc.contributor.authorOhashi, Nen_US
dc.contributor.authorSu, YNen_US
dc.contributor.authorLim, Jen_US
dc.date.accessioned2012-11-26T08:48:10Z-
dc.date.available2012-11-26T08:48:10Z-
dc.date.issued2004en_US
dc.identifier.citationAstrophysical Journal Letters, 2004, v. 616 n. 1 II, p. L19-L22en_US
dc.identifier.issn2041-8205en_US
dc.identifier.urihttp://hdl.handle.net/10722/174925-
dc.description.abstractSubmillimeter Array (SMA) observations of the high-mass star-forming region IRAS 18089-1732 in the 1 mm and 850 μm band with 1 GHz bandwidth reveal a wealth of information. We present the observations of 34 lines from 16 different molecular species. Most molecular line maps show significant contributions from the outflow, and only a few molecules are confined to the inner core. We present and discuss the molecular line observations and outline the unique capabilities of the SMA for future imaging line surveys at high spatial resolution.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.subjectAstrochemistryen_US
dc.subjectLine: Identificationen_US
dc.subjectStars: Formationen_US
dc.subjectSubmillimeteren_US
dc.subjectTechniques: Interferometricen_US
dc.subjectTechniques: Spectroscopicen_US
dc.titleSubmillimeter Array multiline observations of the massive star-forming region IRAS 18089-1732en_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-s2.0-12344284207en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-12344284207&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume616en_US
dc.identifier.issue1 IIen_US
dc.identifier.spageL19en_US
dc.identifier.epageL22en_US
dc.publisher.placeUnited Kingdomen_US
dc.identifier.scopusauthoridBeuther, H=10140586700en_US
dc.identifier.scopusauthoridZhang, Q=8602636100en_US
dc.identifier.scopusauthoridHunter, TR=35394114700en_US
dc.identifier.scopusauthoridSridharan, TK=6701592129en_US
dc.identifier.scopusauthoridZhao, JH=7410310692en_US
dc.identifier.scopusauthoridSollins, P=7004013438en_US
dc.identifier.scopusauthoridHo, PTP=7402211489en_US
dc.identifier.scopusauthoridLiu, SY=7409459358en_US
dc.identifier.scopusauthoridOhashi, N=7202558313en_US
dc.identifier.scopusauthoridSu, YN=35753955800en_US
dc.identifier.scopusauthoridLim, J=7403453870en_US

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