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Apparent-Double SiO Maser Sources

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dc.contributor.authorDeguchi, Shuji
dc.contributor.authorFujii, Takahiro
dc.contributor.authorIzumiura, Hideyuki
dc.contributor.authorMatsumoto, Shigeru
dc.contributor.authorNakada, Y
dc.contributor.authorWood, Peter R
dc.contributor.authorYamamura, I
dc.date.accessioned2015-12-13T23:40:26Z
dc.date.issued1999
dc.date.updated2015-12-12T09:29:06Z
dc.description.abstractDuring the course of a SiO maser survey of galactic disk IRAS sources at 43 GHz, we found two cases of doubly peaked SiO maser sources in the 40″ half-power beam of the Nobeyama 45-m telescope. The double peaks in the spectra of these sources (IRAS 1801
dc.identifier.issn0004-6264
dc.identifier.urihttp://hdl.handle.net/1885/94464
dc.publisherAstronomical Society of Japan
dc.sourcePublications of the Astronomical Society of Japan
dc.subjectKeywords: Infrared: Sources; Masers; Stars: Long-period variables
dc.titleApparent-Double SiO Maser Sources
dc.typeJournal article
local.bibliographicCitation.lastpage361
local.bibliographicCitation.startpage355
local.contributor.affiliationDeguchi, Shuji, National Astronomical Observatory of Japan
local.contributor.affiliationFujii, Takahiro, University of Tokyo
local.contributor.affiliationIzumiura, Hideyuki, National Astronomical Observatory of Japan
local.contributor.affiliationMatsumoto, Shigeru, University of Tokyo
local.contributor.affiliationNakada, Y, University of Tokyo
local.contributor.affiliationWood, Peter R, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationYamamura, I, University of Tokyo
local.contributor.authoruidWood, Peter R, u7900259
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub24059
local.identifier.citationvolume51
local.identifier.scopusID2-s2.0-0033241575
local.type.statusPublished Version

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