The X-ray position and optical counterpart of the accretion-powered millisecond pulsar XTE J1814-338

Astrophysical Journal

Volumn 627, Issue 2 I, 2005, Pages 910-914

  Krauss, Miriam I ^a   Wang, Zhongxiang ^a   Dullighan, Allyn ^a   Juett, Adrienne M ^a,e   Kaplan, David L ^a   Chakrabarty, Deepto ^a   Van Kerkwijk, Marten H ^b   Steeghs, Danny ^c   Jonker, Peter G ^c,f   Markwardt, Craig B ^d,g  

^a MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^b UNIVERSITY OF TORONTO   (Canada)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d Bldg 142   (United States)

^e UNIVERSITY OF VIRGINIA   (United States)

^f SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^g NASA GODDARD SPACE FLIGHT CENTER   (United States)

Author keywords

Binaries: close; Pulsars: individual (XTE J1814 338); Stars: neutron; X rays: binaries

Indexed keywords

EID: 25844528102     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/430595     Document Type: Article

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