Abundances of the elements He to Ni in the atmosphere of Sirius A

Astronomy and Astrophysics

Volumn 528, Issue , 2011, Pages

  Landstreet, J D ^a,b  

^a ARMAGH OBSERVATORY   (United Kingdom)

^b UNIVERSITY OF WESTERN ONTARIO   (Canada)

Author keywords

stars: abundances; stars: chemically peculiar; stars: early type; stars: evolution; stars: individual: HD 48915; Ultraviolet: stars

Indexed keywords

STARS: ABUNDANCES; STARS: CHEMICALLY PECULIAR; STARS: EARLY-TYPE; STARS: EVOLUTION; STARS: INDIVIDUAL: HD 48915; ULTRAVIOLET: STARS;

ATMOSPHERIC TURBULENCE; BARIUM; CHEMICAL ANALYSIS; CHEMICAL ELEMENTS; FADING (RADIO); FORECASTING; GRAVITATION; SIGNAL TO NOISE RATIO; SPECTROSCOPY; STARS; STRONTIUM; ZIRCONIUM;

AMERICIUM;

EID: 79952649555     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201016259     Document Type: Article

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