Detection of highly-ionized carbon and nitrogen emission lines from the cygnus loop supernova remnant with the Suzaku observatory

Publications of the Astronomical Society of Japan

Volumn 59, Issue 1 SPEC. ISS., 2007, Pages

  Miyata, Emi ^a   Katsuda, Satoru ^a   Tsunemi, Hiroshi ^a   Hughes, John P ^b   Kokubun, Motohide ^c   Porter, F Scott ^d  

^a OSAKA UNIVERSITY   (Japan)

^b RUTGERS UNIVERSITY   (United States)

^c UNIVERSITY OF TOKYO   (Japan)

^d NASA GODDARD SPACE FLIGHT CENTER   (United States)

Author keywords

ISM: abundances; ISM: individual (Cygnus Loop); ISM: supernova remnants; X rays: ISM

Indexed keywords

CARBON; CCD CAMERAS; ELECTROMAGNETIC WAVE EMISSION; IONIZATION; NITROGEN; SPECTRUM ANALYSIS; SPECTRAL RESOLUTION;

CARBON EMISSIONS; CYGNUS LOOP; EMISSION LINES; HIGHLY-IONIZED; ISM: ABUNDANCE; ISM: INDIVIDUAL (CYGNI LOOP); ISM: INDIVIDUALS; ISM: SUPERNOVA REMNANTS; SUPERNOVA REMNANTS; X RAYS: ISM;

SPECTRAL RESOLUTION; CARBON;

EID: 34047108588     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/59.sp1.s163     Document Type: Article

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