File Download

There are no files associated with this item.

  Links for fulltext
     (May Require Subscription)
Supplementary

Article: SiO maser survey of southern IRAS sources

TitleSiO maser survey of southern IRAS sources
Authors
KeywordsGalaxy: Kinematics And Dynamics
Galaxy: Structure
Radio Lines: Stars
Stars: Late-Type
Issue Date2001
PublisherNihon Tenmon Gakkai. The Journal's web site is located at http://www.asj.or.jp/pasj/
Citation
Publications Of The Astronomical Society Of Japan, 2001, v. 53 n. 2, p. 305-314 How to Cite?
AbstractWe have surveyed 163 southern IRAS sources in the SiO J = 2-1 v = 1 maser line at 86 GHz, obtaining 38 (22 new and 16 previously known) detections. These detections include 6 stars not previously detected in OH 1612 MHz surveys, and 4 sources assigned incorrect OH radial velocities. The distance reachable in this survey turned out to be about 4 kpc. The local velocity dispersion near the Sun were found to be approximately 30 km s-1 for these IRAS/SiO sources. A relatively high concentration of the SiO detected sources were found at the area 320° < l < 340° (toward "Norma tangent"). The estimated distances for these sources suggest that this concentration is spread between 2 and 6 kpc from the Sun, peaking on the Scutum-Crux arm.
Persistent Identifierhttp://hdl.handle.net/10722/174810
ISSN
2015 Impact Factor: 1.961
2015 SCImago Journal Rankings: 0.804
References

 

DC FieldValueLanguage
dc.contributor.authorDeguchi, Sen_US
dc.contributor.authorNakashima, JIen_US
dc.contributor.authorBalasubramanyam, Ren_US
dc.date.accessioned2012-11-26T08:47:35Z-
dc.date.available2012-11-26T08:47:35Z-
dc.date.issued2001en_US
dc.identifier.citationPublications Of The Astronomical Society Of Japan, 2001, v. 53 n. 2, p. 305-314en_US
dc.identifier.issn0004-6264en_US
dc.identifier.urihttp://hdl.handle.net/10722/174810-
dc.description.abstractWe have surveyed 163 southern IRAS sources in the SiO J = 2-1 v = 1 maser line at 86 GHz, obtaining 38 (22 new and 16 previously known) detections. These detections include 6 stars not previously detected in OH 1612 MHz surveys, and 4 sources assigned incorrect OH radial velocities. The distance reachable in this survey turned out to be about 4 kpc. The local velocity dispersion near the Sun were found to be approximately 30 km s-1 for these IRAS/SiO sources. A relatively high concentration of the SiO detected sources were found at the area 320° < l < 340° (toward "Norma tangent"). The estimated distances for these sources suggest that this concentration is spread between 2 and 6 kpc from the Sun, peaking on the Scutum-Crux arm.en_US
dc.languageengen_US
dc.publisherNihon Tenmon Gakkai. The Journal's web site is located at http://www.asj.or.jp/pasj/en_US
dc.relation.ispartofPublications of the Astronomical Society of Japanen_US
dc.subjectGalaxy: Kinematics And Dynamicsen_US
dc.subjectGalaxy: Structureen_US
dc.subjectRadio Lines: Starsen_US
dc.subjectStars: Late-Typeen_US
dc.titleSiO maser survey of southern IRAS sourcesen_US
dc.typeArticleen_US
dc.identifier.emailNakashima, JI: junichi@hku.hken_US
dc.identifier.authorityNakashima, JI=rp00764en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.scopuseid_2-s2.0-0035626315en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-0035626315&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume53en_US
dc.identifier.issue2en_US
dc.identifier.spage305en_US
dc.identifier.epage314en_US
dc.publisher.placeJapanen_US
dc.identifier.scopusauthoridDeguchi, S=7006314159en_US
dc.identifier.scopusauthoridNakashima, JI=35485342300en_US
dc.identifier.scopusauthoridBalasubramanyam, R=14018985200en_US

Export via OAI-PMH Interface in XML Formats


OR


Export to Other Non-XML Formats