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Near-IR Observations of IRAS Sources with SiO Masers at the Inner Galactic Bulge

dc.contributor.authorDeguchi, Shuji
dc.contributor.authorFujii, Takahiro
dc.contributor.authorMatsumoto, Shigeru
dc.contributor.authorNakashima, Jun-Ichi
dc.contributor.authorWood, Peter R
dc.date.accessioned2015-12-13T23:16:28Z
dc.date.issued2001
dc.date.updated2015-12-12T08:48:15Z
dc.description.abstractNear-infrared photometric observations in the J-, H-, and K-bands have been made for 86 IRAS sources toward the inner Galactic bulge (|l| < 3° and |b| < 3°). SiO maser emission has previously been detected in all of these sources; they are well-confirme
dc.identifier.issn0004-6264
dc.identifier.urihttp://hdl.handle.net/1885/89425
dc.publisherAstronomical Society of Japan
dc.sourcePublications of the Astronomical Society of Japan
dc.subjectKeywords: Galaxy: bulge; Infrared: sources; Stars: kinematics; Stars: long-period variables; Stars: mass loss
dc.titleNear-IR Observations of IRAS Sources with SiO Masers at the Inner Galactic Bulge
dc.typeJournal article
local.bibliographicCitation.lastpage304
local.bibliographicCitation.startpage293
local.contributor.affiliationDeguchi, Shuji, National Astronomical Observatory of Japan
local.contributor.affiliationFujii, Takahiro, University of Tokyo
local.contributor.affiliationMatsumoto, Shigeru, University of Tokyo
local.contributor.affiliationNakashima, Jun-Ichi, National Astronomical Observatory of Japan
local.contributor.affiliationWood, Peter R, College of Physical and Mathematical Sciences, ANU
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.ariespublicationMigratedxPub19441
local.identifier.citationvolume53
local.identifier.scopusID2-s2.0-0035645758
local.type.statusPublished Version

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