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Volumn 662, Issue 2 I, 2007, Pages 1167-1172

The hard X-ray tails in neutron star low-mass X-ray binaries: BeppoSAX observations and possible theoretical explanation of the case of GX 17+2

Author keywords

Accretion, accretion disks; Stars: neutron; X rays: binaries

Indexed keywords


EID: 34547253733     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/516707     Document Type: Article
Times cited : (33)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.