The X-ray spectrum of the classical TTauri star TW Hydrae observed by LETGS aboard Chandra

Astronomy and Astrophysics

Volumn 505, Issue 2, 2009, Pages 755-762

  Raassen, A J J ^a,b  

^a SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^b UNIVERSITY OF AMSTERDAM   (Netherlands)

Author keywords

Stars: coronae; Stars: individual: TW Hya; Techniques: spectroscopic

Indexed keywords

BLACKBODY COMPONENTS; CHANDRA; CORONAL PLASMAS; CORONAL TEMPERATURES; ELECTRON DENSITIES; ELEMENTAL ABUNDANCE; GAUSSIAN LINE; INTER-COMBINATION LINE; IONISATION EQUILIBRIA; LATE-TYPE; LINE FEATURES; OPTICALLY THIN PLASMAS; PLASMA PROPERTIES; RESPONSE MATRICES; STARS: CORONAE; STARS: INDIVIDUAL: TW HYA; STRONG ENHANCEMENT; TECHNIQUES: SPECTROSCOPIC; TW HYDRAE; WAVELENGTH RANGES; X RAY SPECTRUM; X-RAY LUMINOSITY;

CARRIER CONCENTRATION; ELECTRON DENSITY MEASUREMENT; ELECTRON TEMPERATURE; EMISSION SPECTROSCOPY; INFORMATION SCIENCE; NEON; PLASMAS; STARS; X RAY ANALYSIS; X RAY SPECTROGRAPHS;

ELECTRONS;

EID: 70349954737     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811374     Document Type: Article

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