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Optical Counterpart of the X-ray Transient RX J0117.6-7330: Spectroscopy and Photometry

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dc.contributor.authorSoria, Roberto
dc.date.accessioned2015-12-13T23:40:30Z
dc.date.available2015-12-13T23:40:30Z
dc.date.issued1999
dc.date.updated2015-12-12T09:29:19Z
dc.description.abstractWe conducted spectroscopic and photometric observations of the optical companion of the X-ray transient RX J0117·6-7330 in the Small Magellanic Cloud, during a quiescent state. The primary star is identified as a B0·5 IIIe with a mass M* = (18 ± 2)M⊙
dc.identifier.issn1323-3580
dc.identifier.urihttp://hdl.handle.net/1885/94499
dc.publisherCSLI Publications
dc.sourcePublications of the Astronomical Society of Australia
dc.subjectKeywords: Galaxies: Magellanic Clouds; Stars: individual (RX J0117·6-7330); X-ray: binaries
dc.titleOptical Counterpart of the X-ray Transient RX J0117.6-7330: Spectroscopy and Photometry
dc.typeJournal article
local.bibliographicCitation.issue2
local.bibliographicCitation.lastpage151
local.bibliographicCitation.startpage147
local.contributor.affiliationSoria, Roberto, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidSoria, Roberto, u4018394
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub24098
local.identifier.citationvolume16
local.identifier.scopusID2-s2.0-0033437353
local.type.statusPublished Version

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