A Be star with a low nitrogen abundance in the SMC cluster NGC 330

Astronomy and Astrophysics

Volumn 438, Issue 1, 2005, Pages 265-271

  Lennon, D J ^a   Lee, J K ^b   Dufton, P L ^b   Ryans, R S I ^b  

^a ISAAC NEWTON GROUP OF TELESCOPES   (Spain)

^b QUEEN'S UNIVERSITY BELFAST   (United Kingdom)

Author keywords

Galaxies: individual: Small Magellanic Cloud; Stars: abundances; Stars: early type; Stars: emission line, Be

Indexed keywords

CLOUDS; GALAXIES; NITROGEN; ROTATION; SILICON; SPECTROSCOPIC ANALYSIS;

GALAXIES: INDIVIDUAL: SMALL MAGELLANIC CLOUD; STARS: ABUNDANCES; STARS: EARLY-TYPE; STARS: EMISSION-LINE, BE;

ASTROPHYSICS;

EID: 23044486690     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041653     Document Type: Article

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