Equivalent width, shape and proper motion of the iron fluorescent line emission from molecular clouds as an indicator of the illuminating source X-ray flux history

Monthly Notices of the Royal Astronomical Society

Volumn 297, Issue 4, 1998, Pages 1279-1291

  Sunyaev, R ^a,b   Churazov, E ^a,b  

^a MPI für Astrophvsik   (Germany)

^b Russian Academy of Sciences   (Russian Federation)

Author keywords

Galaxy: centre; ISM: individual: Sgr B; Line: formation; X rays: general

Indexed keywords

ANGULAR DISTRIBUTION; IRON; WAVEFRONTS; X RAY OPTICS;

EQUIVALENT WIDTH; GALAXY CENTER; GIANT MOLECULAR CLOUDS; ISM: INDIVIDUAL: SGR B; ISM: INDIVIDUALS; LINE FORMATIONS; MOLECULAR CLOUDS; PROPER MOTION; SHAPE MOTION; X-RAY GENERAL;

FLUORESCENCE;

EID: 0000293142     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01684.x     Document Type: Article

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