Swift monitoring of the new accreting millisecond X-ray pulsar IGR J17511-3057 in outburst

Astronomy and Astrophysics

Volumn 509, Issue 1, 2010, Pages

  Bozzo, E ^a   Ferrigno, C ^a,b   Falanga, M ^c   Campana, S ^d   Kennea, J A ^e   Papitto, A ^f,g  

^a UNIVERSITY OF GENEVA   (Switzerland)

^b UNIVERSITY OF TÜBINGEN   (Germany)

^c INTERNATIONAL SPACE SCIENCE INSTITUTE   (Switzerland)

^d INAF OSSERVATORIO ASTRONOMICO DI BRERA   (Italy)

^e PENNSYLVANIA STATE UNIVERSITY   (United States)

^f UNIVERSITY OF CAGLIARI   (Italy)

^g INAF OSSERVATORIO ASTRONOMICO DI CAGLIARI   (Italy)

Author keywords

Binaries pulsars; IGRJ17511 3057; Individual; X rays

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; HELIUM;

GALACTIC BULGE; HELIUM BURST; MILLISECOND PULSARS; POWER-LAW COMPONENTS; RECURRENCE TIME; SPECTRAL PROPERTIES; UPPER LIMITS; X-RAY BURSTS; X-RAY FLUX; X-RAY PULSARS;

X RAYS;

EID: 76349118751     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913517     Document Type: Article

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