Exploring the X-ray emission properties of the supernova remnant G67.7+1.8 and its central X-ray sources

Astronomy and Astrophysics

Volumn 494, Issue 3, 2009, Pages 1005-1012

  Hui, C Y ^a   Becker, W ^a  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

Author keywords

ISM: supernova remnants; Stars: neutron; Stars: supernovae: individual: G67.7+1.8; X rays: stars

Indexed keywords

CALCIUM; ELECTROMAGNETIC WAVE EMISSION; EMISSION SPECTROSCOPY; INFORMATION SCIENCE; MAGNESIUM; SCANDIUM; STARS; SULFUR; X RAY OPTICS;

A THERMALS; ANGULAR RESOLUTIONS; ARC STRUCTURES; CHANDRA; EMISSION LINES; GAUSSIAN EMISSIONS; HIGHLY-IONIZED; ISM: SUPERNOVA REMNANTS; LINE FEATURES; POINT SOURCES; RADIO WAVELENGTHS; STARS: NEUTRON; STARS: SUPERNOVAE: INDIVIDUAL: G67.7+1.8; SUPERNOVA REMNANTS; X-RAY EMISSIONS; X-RAY MORPHOLOGIES; X-RAY OBSERVATORIES; X-RAY SOURCES; X-RAY SPECTRUM; X-RAYS: STARS;

X RAYS;

EID: 60349116256     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810789     Document Type: Article

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