Understanding the atmospheric structure of T Tauri stars - I. Improved atomic physics applied to IUE data of BP Tauri

Monthly Notices of the Royal Astronomical Society

Volumn 307, Issue 4, 1999, Pages 895-908

  Brooks, D H ^a   Costa, V M ^a   Lago, M T V T ^a   Lanzafame, A C ^b  

^a CENTRO DE ASTROFÍSICA   (Portugal)

^b UNIVERSITY OF CATANIA   (Italy)

Author keywords

Atomic data; Atomic processes; Methods: data analysis; Stars: pre main sequence; Techniques: spectroscopic; Ultraviolet: stars

Indexed keywords

ATMOSPHERIC STRUCTURE; ATOMS; SPECTROSCOPIC ANALYSIS; STARS;

ASTROPHYSICAL PLASMA; ATOMIC DATA; ATOMIC PROCESS; LABORATORY PLASMA; METHODS. DATA ANALYSIS; PROPERTY; STARS: PRE-MAIN SEQUENCE; T TAURI STARS; TECHNIQUES: SPECTROSCOPIC; ULTRAVIOLET: STARS;

ULTRAVIOLET SPECTROSCOPY;

EID: 0042026110     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1999.02668.x     Document Type: Article

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