A long-period, violently variable X-ray source in a young supernova remnant

Science

Volumn 313, Issue 5788, 2006, Pages 814-817

  De Luca, A ^a   Caraveo, P A ^a   Mereghetti, S ^a   Tiengo, A ^a   Bignami, G F ^b,c  

^a INAF IASF MILANO   (Italy)

^b IRAP   (France)

^c UNIVERSITY OF PAVIA   (Italy)

Author keywords

[No Author keywords available]

Indexed keywords

ASTRONOMICAL SATELLITES; ASTRONOMY; MODULATION; X RAY ANALYSIS;

NEUTRON STARS; SUPERNOVA EXPLOSIONS; X-RAY BINARY;

SPACE RESEARCH;

COSMOLOGY; X-RAY;

ARTICLE; COSMOLOGICAL PHENOMENA; COSMOS; ENERGY; INFRARED RADIATION; LUMINANCE; NEUTRON; PRIORITY JOURNAL; X RAY;

EID: 33747107059     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1129185     Document Type: Article

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31. The XMM-Newton data analysis is supported by the Italian Space Agency (ASI) through contract ASI/INAF 1/023/05/0. A.D.L. and A.T. acknowledge an A5I fellowship.