Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | 박일흥 | - |
dc.date.accessioned | 2016-08-28T11:08:00Z | - |
dc.date.available | 2016-08-28T11:08:00Z | - |
dc.date.issued | 2008 | - |
dc.identifier.issn | 2041-8205 | - |
dc.identifier.other | OAK-13240 | - |
dc.identifier.uri | https://dspace.ewha.ac.kr/handle/2015.oak/229263 | - |
dc.description.abstract | The spin parameter of the black hole in M33 X-7 has recently been measured to be a * p 0.77 ± 0.05. It has been proposed that the spin of the 15.65 M⊙ black hole is natal. We show that this is not a viable evolutionary path given the observed binary orbital period of 3.45 days since the explosion that would produce a black hole with the cited spin parameter and orbital period would disrupt the binary. Furthermore, we show that the system has to be evolved through the hypercritical mass transfer of-5 M⊙ from the secondary star to the black hole. © 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A. | - |
dc.language | English | - |
dc.title | The case for hypercritical accretion in m33 x-7 | - |
dc.type | Article | - |
dc.relation.issue | 1 PART 2 | - |
dc.relation.volume | 689 | - |
dc.relation.index | SCI | - |
dc.relation.index | SCIE | - |
dc.relation.index | SCOPUS | - |
dc.relation.startpage | L9 | - |
dc.relation.lastpage | L12 | - |
dc.relation.journaltitle | Astrophysical Journal Letters | - |
dc.identifier.doi | 10.1086/593977 | - |
dc.identifier.wosid | WOS:000262733800003 | - |
dc.identifier.scopusid | 2-s2.0-67649646256 | - |
dc.author.google | Mendez E.M. | - |
dc.author.google | Brown G.E. | - |
dc.author.google | Lee C.-H. | - |
dc.author.google | Park I.H. | - |
dc.contributor.scopusid | 박일흥(7403243322;57199842780) | - |
dc.date.modifydate | 20230616163100 | - |