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Be/X-ray binaries as the progenitors of the supergiant fast X-ray transients IGR J18483-0311 and IGR J11215-5952
Liu, Q. Z.1,2; Chaty, S.2; Yan, J. Z.1,2
2011-08-01
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
Volume415Issue:4Pages:3349-3353
AbstractThe relation between the spin period (P-s) and the orbital period (P-o) in high-mass X-ray binaries is investigated. Be/X-ray binaries and SG/X-ray binaries occupy different areas in the Corbet diagram. The supergiant fast X-ray transients, IGR J18483-0311 and IGR J11215-5952, however, fall into the area occupied by Be/X-ray binaries. After excluding the other evolution scenarios, we find that the positions of the two supergiant fast X-ray transients in the diagram can be interpreted by being the descendants of O-emission X-ray binaries, i.e. the supergiant stars in these systems formed from O-type emission line stars instead of normal main-sequence stars. Therefore, we suggest that there are two types of SG/X-ray binaries: the first one is directly evolved from OB-type main-sequence star and neutron star systems without accretion history, and the other evolved from Be/X-ray binaries with accretion history.
KeywordBinaries: Close Pulsars: Individual: Igr J18483-0311 Pulsars: Individual: Igr J11215-5952 X-rays: Binaries
Subject AreaAstronomy & Astrophysics
WOS HeadingsScience & Technology ; Physical Sciences
DOI10.1111/j.1365-2966.2011.18949.x
WOS KeywordMAGNETIC-FIELD DECAY ; STELLAR WINDS ; NEUTRON-STAR ; 2S 0114+650 ; SPIN ; PARAMETERS ; ACCRETION ; PULSARS ; SIMULATIONS ; OUTBURST
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000294204900033
Citation statistics
Cited Times:15[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/4538
Collection宇宙伽马暴、中子星及相关物理研究团组
Affiliation1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
2.Univ Paris Diderot, Lab AIM, CEA DSM, CNRS,IRFU SAp,Ctr Saclay, F-91191 Gif Sur Yvette, France
Recommended Citation
GB/T 7714
Liu, Q. Z.,Chaty, S.,Yan, J. Z.. Be/X-ray binaries as the progenitors of the supergiant fast X-ray transients IGR J18483-0311 and IGR J11215-5952[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2011,415(4):3349-3353.
APA Liu, Q. Z.,Chaty, S.,&Yan, J. Z..(2011).Be/X-ray binaries as the progenitors of the supergiant fast X-ray transients IGR J18483-0311 and IGR J11215-5952.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,415(4),3349-3353.
MLA Liu, Q. Z.,et al."Be/X-ray binaries as the progenitors of the supergiant fast X-ray transients IGR J18483-0311 and IGR J11215-5952".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 415.4(2011):3349-3353.
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