XMM-Newton observations of the Small Magellanic Cloud: Long term evolution of frequently observed Be/X-ray binaries

Astronomy and Astrophysics

Volumn 491, Issue 3, 2008, Pages 841-849

  Eger, P ^a   Haberl, F ^a  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

Author keywords

Galaxies: individual: Small Magellanic Cloud; Galaxies: stellar content; Stars: emission line, Be; Stars: neutron; X rays: binaries

Indexed keywords

BAYESIAN NETWORKS; ELECTROMAGNETIC WAVES; EMISSION SPECTROSCOPY; FOURIER ANALYSIS; FOURIER TRANSFORMS; GALAXIES; MAXIMUM LIKELIHOOD ESTIMATION; OBSERVATORIES; STARS; X RAY ANALYSIS; X RAY SPECTROGRAPHS; X RAYS;

GALAXIES: INDIVIDUAL: SMALL MAGELLANIC CLOUD; GALAXIES: STELLAR CONTENT; STARS: EMISSION-LINE, BE; STARS: NEUTRON; X-RAYS: BINARIES;

X RAY CAMERAS;

EID: 57049178507     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810809     Document Type: Article

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