Be/X-ray binaries as the progenitors of the supergiant fast X-ray transients IGR J18483-0311 and IGR J11215-5952

CORC > 紫金山天文台 > 中国科学院紫金山天文台 > 宇宙伽马暴、中子星及相关物理研究团组

	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
刊名	MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
	2011-08-01
卷号	415 期号:4 页码:3349-3353
关键词	binaries: close pulsars: individual: IGR J18483-0311 pulsars: individual: IGR J11215-5952 X-rays: binaries
ISSN号	0035-8711
英文摘要	The 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.
学科主题	Astronomy & Astrophysics
WOS标题词	Science & Technology ; Physical Sciences
类目[WOS]	Astronomy & Astrophysics
研究领域[WOS]	Astronomy & Astrophysics
关键词[WOS]	MAGNETIC-FIELD DECAY ; STELLAR WINDS ; NEUTRON-STAR ; 2S 0114+650 ; SPIN ; PARAMETERS ; ACCRETION ; PULSARS ; SIMULATIONS ; OUTBURST
收录类别	SCI
语种	英语
WOS记录号	WOS:000294204900033
公开日期	2012-08-07
内容类型	期刊论文
源URL	[http://libir.pmo.ac.cn/handle/332002/4538]
专题	紫金山天文台_宇宙伽马暴、中子星及相关物理研究团组
作者单位	1.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
推荐引用方式 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.