The peculiar cluster HS 327 in the large Magellanic Cloud: Can OH/IR stars and carbon stars be twins?

Astronomy and Astrophysics

Volumn 368, Issue 1, 2001, Pages 239-249

  Van Loon, J Th ^a   Zijlstra, A A ^b   Kaper, L ^c   Gilmore, G F ^a   Loup, C ^d   Blommaert, J A D L ^e  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^b UNIVERSITY OF MANCHESTER   (United Kingdom)

^c UNIVERSITY OF AMSTERDAM   (Netherlands)

^d INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^e EUROPEAN SPACE AGENCY   (Spain)

Author keywords

Infrared: stars; Open clusters and associations: general Magellanic Clouds; Stars: AGB and post AGB; Stars: carbon; Stars: evolution

Indexed keywords

EID: 0035264282     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20000529     Document Type: Article

References (41)