Hydrogen-like nitrogen radio line from hot interstellar and warm-hot intergalactic gas

Astronomy Letters

Volumn 33, Issue 2, 2007, Pages 67-79

  Sunyaev, R A ^a,b   Docenko, D O ^a  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b Russian Academy of Sciences ^*  (Russian Federation)

Author keywords

Hyperfine structure; Intergalactic gas; Radio lines; Supernova remnants

Indexed keywords

EID: 33847182442     PISSN: 10637737     EISSN: None     Source Type: Journal    
DOI: 10.1134/S1063773707020016     Document Type: Article

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