Variability of the H2O maser associated with the M-supergiant S persei

Astronomy and Astrophysics

Volumn 437, Issue 1, 2005, Pages 127-133

  Lekht, E E ^a,b   Rudnitskij, G M ^b   Mendoza Torres, J E ^a   Tolmachev, A M ^c  

^a INSTITUTO NACIONAL DE ASTROFÍSICA   (Mexico)

^b MOSCOW STATE UNIVERSITY   (Russian Federation)

^c LEBEDEV PHYSICAL INSTITUTE   (Russian Federation)

Author keywords

Circumstellar matter; Masers; Stars: AGB and post AGB; Stars: late type; Stars: mass loss; Stars: supergiants

Indexed keywords

CORRELATION METHODS; DATABASE SYSTEMS; HYDROGEN; INFRARED RADIATION; OPTICAL PROPERTIES; OSCILLATIONS; SPECTRUM ANALYSIS; VAPORS; VELOCITY MEASUREMENT; WATER;

CIRCUMSTELLAR MATTER; STARS: AGB AND POST-AGB; STARS: LATE-TYPE; STARS: MASS-LOSS; STARS: SUPERGIANTS;

MASERS;

EID: 21244452827     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20052635     Document Type: Article

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