XMM-Newton observation of the persistent Be/NS X-ray binary pulsar RX J1037.5-5647 in a low luminosity state

Astronomy and Astrophysics

Volumn 505, Issue 3, 2009, Pages 947-954

  La Palombara, N ^a   Sidoli, L ^a   Esposito, P ^a,b   Tiengo, A ^a   Mereghetti, S ^a  

^a INAF IASF MILANO   (Italy)

^b INFN SEZIONE DI PAVIA   (Italy)

Author keywords

Accretion, accretion disks; Stars: emission line, Be; Stars: pulsars: individual: LS 1698; X rays: binaries; X rays: individuals: RX J1037.5 5647

Indexed keywords

ACCRETION, ACCRETION DISKS; STARS: EMISSION-LINE, BE; STARS: PULSARS: INDIVIDUAL: LS 1698; X-RAYS: BINARIES; X-RAYS: INDIVIDUALS: RX J1037.5-5647;

DISKS (MACHINE COMPONENTS); DISKS (STRUCTURAL COMPONENTS); LUMINANCE; OBSERVATORIES; POWER SPECTRUM; SPECTRUM ANALYSIS; SPECTRUM ANALYZERS; STARS;

X RAYS;

EID: 70350223729     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912538     Document Type: Article

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