G359.95-0.04: An energetic pulsar candidate near Sgr A

Monthly Notices of the Royal Astronomical Society

Volumn 367, Issue 3, 2006, Pages 937-944

  Wang, Q D ^a,b   Lu, F J ^a,c   Gotthelf, E V ^d  

^a UNIVERSITY OF MASSACHUSETTS   (United States)

^b INSTITUTE FOR ADVANCED STUDY   (United States)

^c INSTITUTE OF HIGH ENERGY PHYSICS   (China)

^d Columbia University ^*  (United States)

Author keywords

Pulsars: general; Supernova remnants; X rays: individual: G359.95 0.04, Sgr A*, IRS 13

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; SUPERNOVAE; TELLURIUM COMPOUNDS;

GALACTIC CENTER; NONTHERMAL; POWER LAW SPECTRUM; PULSAR WIND NEBULA; PULSARS: GENERAL; STELLAR COMPLEXES; SUPERNOVA REMNANTS; X-RAY CHARACTERISTICS; X-RAY: INDIVIDUAL: G359.95-0.04, SGR A*, IRS 13; X-RAYS: INDIVIDUAL;

PULSARS;

EID: 33645415701     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.09998.x     Document Type: Article

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