A state change in the low-mass X-ray binary XSS J12270-4859

Monthly Notices of the Royal Astronomical Society

Volumn 441, Issue 2, 2014, Pages 1825-1830

  Bassa, C G ^a   Patruno, A ^a,b   Hessels, J W T ^a,c   Keane, E F ^d,e   Monard, B ^f   Mahony, E K ^a   Bogdanov, S ^g   Corbel, S ^h   Edwards, P G ⁱ   Archibald, A M ^a   Janssen, G H ^a   Stappers, B W ^j   Tendulkar, S ^k  

^a ASTRON   (Netherlands)

^b LEIDEN UNIVERSITY   (Netherlands)

^c UNIVERSITY OF AMSTERDAM   (Netherlands)

^d SWINBURNE UNIVERSITY OF TECHNOLOGY   (Australia)

^e ARC CENTRE OF EXCELLENCE FOR ALL SKY ASTROPHYSICS CAASTRO   (Australia)

^f Kleinkaroo Observatory   (South Africa)

^g Och Spine at New York Presbyterian Hospitals   (United States)

^h CEA SACLAY   (France)

ⁱ CSIRO   (Australia)

^j UNIVERSITY OF MANCHESTER   (United Kingdom)

^k CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

more..

Author keywords

Binaries; General stars; Individual; Neutron X rays; XSS J12270 4859 stars

Indexed keywords

BINARY; GENERAL - STARS; INDIVIDUAL; LOW-MASS X-RAY BINARIES; MILLISECOND PULSARS; NEUTRON-X-RAY; OPTICAL-; RADIO PULSARS; STATES CHANGE; XSS J12270-4859-STAR;

PULSARS;

EID: 84900531313     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1093/mnras/stu708     Document Type: Article

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