Very low luminosities from the accretion-driven millisecond X-ray pulsar SAX J1808.4-3658 during quiescence

Astrophysical Journal

Volumn 571, Issue 1 I, 2002, Pages 429-434

  Wijnands, Rudy ^a   Kuiper, Lucien ^b   In 't Zand, Jean ^b,c   Dotani, Tadayasu ^d   Van der Klis, Michiel ^e   Heise, John ^b  

^a MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^b SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^c UTRECHT UNIVERSITY   (Netherlands)

^d JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

^e UNIVERSITY OF AMSTERDAM   (Netherlands)

Author keywords

Accretion, accretion disks; Stars: individual (SAX J1808.4 3658); Stars: neutron; X rays: stars

Indexed keywords

EID: 0037674706     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/339912     Document Type: Article

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