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Near-Infrared Observations of the IRAS/SiO Sources in the Galactic Bulge: a Large Scale Distribution

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dc.contributor.authorDeguchi, Shuji
dc.contributor.authorFujii, Takahiro
dc.contributor.authorNakashima, Jun-Ichi
dc.contributor.authorWood, Peter R
dc.date.accessioned2015-12-13T23:39:51Z
dc.date.issued2002
dc.date.updated2015-12-12T09:26:53Z
dc.description.abstractNear-infrared photometric obserwttions in the J-, H-, and K-bands were made for 120 IRAS sources toward the Galactic bulge (-10° < l < 15° and |b| < 3°, excluding |l| < 3°). They are well-confirmed, mass-losing late-type stars having accurate radial v
dc.identifier.issn0004-6264
dc.identifier.urihttp://hdl.handle.net/1885/94213
dc.publisherAstronomical Society of Japan
dc.sourcePublications of the Astronomical Society of Japan
dc.subjectKeywords: Galaxies: Milky Way; Infrared: sources; Stars: kinematics; Stars: long-period variables; Stars: mass-loss
dc.titleNear-Infrared Observations of the IRAS/SiO Sources in the Galactic Bulge: a Large Scale Distribution
dc.typeJournal article
local.bibliographicCitation.lastpage734
local.bibliographicCitation.startpage719
local.contributor.affiliationDeguchi, Shuji, National Astronomical Observatory of Japan
local.contributor.affiliationFujii, Takahiro, 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.ariespublicationMigratedxPub23742
local.identifier.citationvolume54
local.identifier.scopusID2-s2.0-0036460631
local.type.statusPublished Version

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