K-shell emission of neutral iron line from sagittarius B2 excited by subrelativistic protons

Publications of the Astronomical Society of Japan

Volumn 63, Issue 3, 2011, Pages 535-541

  Dogiel, Vladimir ^a   Chernyshov, Dmitrii ^a,c   Koyama, Katsuji ^b   Nobukawa, Masayoshi ^a   Cheng, Kwong Sang ^c  

^a LEBEDEV PHYSICAL INSTITUTE   (Russian Federation)

^b KYOTO UNIVERSITY   (Japan)

^c UNIVERSITY OF HONG KONG   (Hong Kong)

Author keywords

Cosmic rays; Galaxy: center; ISM: clouds; X rays: ISM

Indexed keywords

COSMIC RAYS; COSMOLOGY; IRON;

GALACTIC CENTER; GALAXY CENTER; ISM : CLOUDS; K-SHELL EMISSION; KΑ; LINE INTENSITIES; MOLECULAR CLOUDS; SAGITTARIUS B2; TOTAL FLUX; X RAYS: ISM;

CLOUDS;

EID: 79959672812     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/63.3.535     Document Type: Article

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