Late-type giant variables in NGC 6522, LMC and SMC. How do they differ?

Astronomy and Astrophysics

Volumn 427, Issue 3, 2004, Pages 945-958

  Schultheis, M ^a,b   Glass, I S ^c   Cioni, M R ^d  

^a OBSERVATOIRE DE BESANÇON   (France)

^b INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^c SOUTH AFRICAN ASTRONOMICAL OBSERVATORY   (South Africa)

^d EUROPEAN SOUTHERN OBSERVATORY   (Germany)

Author keywords

AGB and post AGB Galaxies; Bulge; Magellanic Clouds Galaxy; Stars

Indexed keywords

CARBON; CLOUDS; GALAXIES; GRAVITATIONAL EFFECTS; MONITORING; PHOTOMETRY; SENSITIVITY ANALYSIS;

AGB AND POST-AGB GALAXIES; MAGELLANIC CLOUD MINI-SURVEY (MCMS); MAGNELLANIC CLOUDS-GALAXY: BULGE; STARS;

ASTROPHYSICS;

EID: 10044283250     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041454     Document Type: Review

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