The intriguing nature of the high-energy gamma ray source XSS J12270-4859

Astronomy and Astrophysics

Volumn 515, Issue 4, 2010, Pages

  De Martino, D ^a   Falanga, M ^b   Bonnet Bidaud, J M ^c   Belloni, T ^d   Mouchet, M ^e   Masetti, N ^f,g   Andruchow, I ^h   Cellone, S A ^h   Mukai, K ^i,j   Matt, G ^k  

^a INAF OSSERVATORIO ASTRONOMICO DI CAPODIMONTE   (Italy)

^b INTERNATIONAL SPACE SCIENCE INSTITUTE   (Switzerland)

^c CEA SACLAY   (France)

^d INAF OSSERVATORIO ASTRONOMICO DI BRERA   (Italy)

^e UNIVERSITÉ PARIS DIDEROT   (France)

^f OBSERVATOIRE DE PARIS   (France)

^g OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^h INSTITUTO DE ASTROFÍSICA DE LA PLATA   (Argentina)

ⁱ NASA GODDARD SPACE FLIGHT CENTER   (United States)

^j UNIVERSITY OF MARYLAND BALTIMORE COUNTY   (United States)

^k ROMA TRE UNIVERSITY   (Italy)

more..

Author keywords

Binaries: close; Stars: individual: 1FGLJ1227.9 4852; Stars: individual: XSS J12270 4859; X rays: binaries

Indexed keywords

ELECTRON SOURCES; HIGH ENERGY PHYSICS; LUMINANCE; PHOTOMETERS; PHOTOMETRY; SPECTROSCOPY; STARS; X RAY ANALYSIS; X RAY SPECTROGRAPHS; X RAYS;

BINARIES: CLOSE; BROAD BANDS; CATACLYSMIC VARIABLES; GAMMA RAY SOURCES; GAMMA RAY SPECTRA; GROUND BASED; HARD X-RAY SOURCES; HIGH ENERGY; HIGH ENERGY GAMMA RAYS; IR BANDS; LARGE AMPLITUDE; LOW-MASS; NEAR-IR; OPTICAL PHOTOMETRY; OPTICAL SPECTRA; ORBITAL PERIODS; POINT SOURCES; POWER LAW INDEX; POWER LAW MODEL; SPECTRAL CHARACTERISTICS; SPECTRAL PROPERTIES; STARS: INDIVIDUAL; TIME-SCALES; TOTAL ENERGY; UV- AND; X RAY BANDS; X RAY BINARIES; X RAY SPECTRUM; X-RAY EMISSION; X-RAY SOURCES; X-RAYS: BINARIES; XMM-NEWTON; XMM-NEWTON OBSERVATIONS;

GAMMA RAYS;

EID: 77953196953     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913802     Document Type: Article

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