A study of the s-process in the carbon-rich post-AGB stars IRAS 06530-0213 and IRAS 08143-4406 on the basis of VLT-UVES spectra

Astronomy and Astrophysics

Volumn 417, Issue 1, 2004, Pages 269-281

  Reyniers, M ^a   Van Winckel, H ^a   Gallino, R ^b,c   Straniero, O ^d  

^a KU LEUVEN   (Belgium)

^b UNIVERSITY OF TURIN   (Italy)

^c MONASH UNIVERSITY   (Australia)

^d INAF OSSERVATORIO ASTRONOMICO DI COLLURANIA   (Italy)

Author keywords

Line: identification; Stars: abundances; Stars: AGB and post AGB; Stars: carbon; Stars: chemically peculiar; Stars: evolution; Stars: individual: IRAS 06530 0213; Stars: individual: IRAS 08143 4406

Indexed keywords

AMORPHOUS MATERIALS; CARBON; INFRARED RADIATION; MORPHOLOGY; NEUTRONS; OPTICAL RESOLVING POWER; SIGNAL TO NOISE RATIO; SILICATES;

IRAS 08143-4406; LINE: IDENTIFICATION; STARS: ABUNDANCES; STARS: AGB AND POST-AGB; STARS: CARBON; STARS: CHEMICALLY PECULIAR; STARS: EVOLUTION; STARS: INDIVIDUAL; STARS: INDIVIDUAL: IRAS 06530-0213;

ASTROPHYSICS;

EID: 1842582858     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20034397     Document Type: Article

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