A possible formation mechanism of the asymmetry in the H2O maser emission line

Astronomy Letters

Volumn 28, Issue 4, 2002, Pages 217-222

  Silant'ev N A ^a,b   Lekht, E E ^a,c   Mendosa Torres, J E ^a   Tolmachev, A M ^d  

^a INSTITUTO NACIONAL DE ASTROFÍSICA   (Mexico)

^b RUSSIAN ACADEMY OF SCIENCES   (Russian Federation)

^c MOSCOW STATE UNIVERSITY   (Russian Federation)

^d LEBEDEV PHYSICAL INSTITUTE   (Russian Federation)

Author keywords

Interstellar molecules; Maser radio sources; Star forming regions

Indexed keywords

EID: 0036544698     PISSN: 10637737     EISSN: None     Source Type: Journal    
DOI: 10.1134/1.1467256     Document Type: Article

References (10)