First spectroscopic analysis of β Scorpii C and β Scorpii e discovery of a new HgMn star in the multiple system β Scorpii

Astronomy and Astrophysics

Volumn 509, Issue 1, 2010, Pages

  Catanzaro, G ^a  

^a INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

Author keywords

Abundances Stars; Chemically peculiar; Individual; Spectroscopic Stars; Stars; Scorpii Binaries

Indexed keywords

CHEMICAL ELEMENTS; HARMONIC ANALYSIS; INTERPLANETARY FLIGHT; MAGNESIUM; MANGANESE; MERCURY (METAL); METAL REFINING; NEON; OXYGEN; PHOSPHORUS; SATELLITES; SPECTROSCOPIC ANALYSIS; SPECTROSCOPY; STRONTIUM; SULFUR; TITANIUM; VELOCITY;

ABUNDANCES - STARS; ATMOSPHERIC PARAMETERS; BALMER LINES; CHEMICALLY PECULIAR; DOPPLER SHIFTS; JUPITERS; LIGHT ELEMENTS; LOCAL THERMODYNAMIC EQUILIBRIUM; METALLIC LINES; MODEL ATMOSPHERE; MULTIPLE SYSTEMS; OPTICAL SPECTROSCOPY; PRINCIPAL COMPONENTS; RADIAL VELOCITY; ROTATIONAL VELOCITY; SOLAR ABUNDANCES; SPECTRAL SYNTHESIS; SPECTROSCOPIC-STARS; TRIPLE SYSTEM;

STARS;

EID: 76349110111     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913332     Document Type: Article

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