The bright unidentifiedγ-ray source 1FGL J1227.9-4852: Can it be associated with a low-mass X-ray binary?

Monthly Notices of the Royal Astronomical Society

Volumn 415, Issue 1, 2011, Pages 235-243

  Hill, A B ^a   Szostek, A ^a,b   Corbel, S ^c   Camilo, F ^d   Corbet, R H D ^e,f   Dubois, R ^g   Dubus, G ^a   Edwards, P G ^h   Ferrara, E C ^e   Kerr, M ^g   Koerding, E ^c   Koziel D ^b   Stawarz, L ^b,i  

^a UNIV GRENOBLE ALPES   (France)

^b JAGIELLONIAN UNIVERSITY   (Poland)

^c UNIVERSITÉ PARIS DIDEROT   (France)

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

^e NASA GODDARD SPACE FLIGHT CENTER   (United States)

^f NATIONAL SPACE SCIENCE AND TECHNOLOGY CENTER   (United States)

^g SLAC NATIONAL ACCELERATOR LABORATORY   (United States)

^h CSIRO   (Australia)

ⁱ JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

Author keywords

Galaxies: active; Gamma rays: general; Pulsars: general; Radio continuum: galaxies; X rays: individual: XSS J12270 4859

Indexed keywords

GALAXIES; PULSARS; RADIO ASTRONOMY; RADIO TELESCOPES; ULTRAVIOLET SPECTROSCOPY;

ENERGY; FOLLOW UP; GALAXIES ACTIVE; GAMMA RAYS: GENERALS; GAMMA-RAYS; LOW-MASS X-RAY BINARIES; PULSARS: GENERAL; RADIO CONTINUUM: GALAXIES; X-RAY: INDIVIDUAL: XSS J12270-4859; X-RAYS: INDIVIDUAL;

GAMMA RAYS;

EID: 79960134138     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.18692.x     Document Type: Article

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