Radio H I and optical absorption-line spectra of an intermediate-velocity cloud in the general direction of the M15 globular cluster

Monthly Notices of the Royal Astronomical Society

Volumn 297, Issue 3, 1998, Pages 849-859

  Kennedy, D C ^a   Bates, B ^a   Keenan, F P ^a   Kemp, S N ^a,b   Ryans, R S I ^a   Davies, R D ^c   Sembach, K R ^d  

^a QUEEN'S UNIVERSITY BELFAST   (United Kingdom)

^b INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^c UNIVERSITY OF MANCHESTER   (United Kingdom)

^d JOHNS HOPKINS UNIVERSITY   (United States)

Author keywords

Globular clusters: individual: M15; ISM: abundances; ISM: clouds; ISM: general; ISM: structure; Stars: individual: HD 203664

Indexed keywords

LIGHT ABSORPTION; SODIUM COMPOUNDS; STARS; VELOCITY;

COLUMN DENSITY; GLOBULAR CLUSTER: INDIVIDUAL: M15; GLOBULAR CLUSTERS: INDIVIDUAL; ISM : CLOUDS; ISM: ABUNDANCE; ISM: STRUCTURE; ISM:GENERAL; LINE SPECTRA; STAR: INDIVIDUAL: HD 203664; STARS: INDIVIDUAL: PROXIMA CENTAURI;

GASES;

EID: 0009231948     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01549.x     Document Type: Article

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