DC Field | Value | Language |
---|---|---|
dc.contributor.author | Seon, KI | ko |
dc.contributor.author | Min, KyoungWook | ko |
dc.contributor.author | Yoshida, K | ko |
dc.contributor.author | Makino, F | ko |
dc.contributor.author | Lewin, WHG | ko |
dc.contributor.author | vanderKlis, M | ko |
dc.contributor.author | vanParadijs, J | ko |
dc.date.accessioned | 2013-02-28T00:34:23Z | - |
dc.date.available | 2013-02-28T00:34:23Z | - |
dc.date.created | 2012-02-06 | - |
dc.date.created | 2012-02-06 | - |
dc.date.created | 2012-02-06 | - |
dc.date.issued | 1997-04 | - |
dc.identifier.citation | ASTROPHYSICAL JOURNAL, v.479, no.1, pp.398 - 407 | - |
dc.identifier.issn | 0004-637X | - |
dc.identifier.uri | http://hdl.handle.net/10203/71767 | - |
dc.description.abstract | We present a detailed analysis of simultaneous Ginga and ROSAT observations of the X-ray burst source 1735-444, during which the source was in an unusually high luminosity state. The source shows the characteristics of an atoll source in the high-intensity (banana state, with a general correlation between intensity and spectral hardness. A blackbody component contributes similar to 15%-20% of the total flux when the conventional two-component model is used to fit the spectra. We also observed a bright burst with radius expansion al this very high luminosity. The burst spectrum could not be described by a simple blackbody model. We discuss possible explanations. | - |
dc.language | English | - |
dc.publisher | UNIV CHICAGO PRESS | - |
dc.title | Results of Ginga/ROSAT simultaneous observation of the X-ray burst source 1735-444 | - |
dc.type | Article | - |
dc.identifier.wosid | A1997WR66000040 | - |
dc.identifier.scopusid | 2-s2.0-21744462109 | - |
dc.type.rims | ART | - |
dc.citation.volume | 479 | - |
dc.citation.issue | 1 | - |
dc.citation.beginningpage | 398 | - |
dc.citation.endingpage | 407 | - |
dc.citation.publicationname | ASTROPHYSICAL JOURNAL | - |
dc.contributor.localauthor | Min, KyoungWook | - |
dc.contributor.nonIdAuthor | Seon, KI | - |
dc.contributor.nonIdAuthor | Yoshida, K | - |
dc.contributor.nonIdAuthor | Makino, F | - |
dc.contributor.nonIdAuthor | Lewin, WHG | - |
dc.contributor.nonIdAuthor | vanderKlis, M | - |
dc.contributor.nonIdAuthor | vanParadijs, J | - |
dc.type.journalArticle | Article | - |
dc.subject.keywordAuthor | binaries, close | - |
dc.subject.keywordAuthor | stars, individual (1735 - 444) | - |
dc.subject.keywordAuthor | X-rays, bursts | - |
dc.subject.keywordAuthor | X-rays, stars | - |
dc.subject.keywordPlus | ACCRETING NEUTRON-STARS | - |
dc.subject.keywordPlus | SUB-HERTZ NOISE | - |
dc.subject.keywordPlus | K LINE EMISSION | - |
dc.subject.keywordPlus | EXOSAT OBSERVATIONS | - |
dc.subject.keywordPlus | GX 17+2 | - |
dc.subject.keywordPlus | OPTICAL VARIABILITY | - |
dc.subject.keywordPlus | RADIUS EXPANSION | - |
dc.subject.keywordPlus | BINARIES | - |
dc.subject.keywordPlus | SPECTRA | - |
dc.subject.keywordPlus | GINGA | - |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.