Modeling CHANDRA low energy transmission grating spectrometer observations of classical novae with PHOENIX I. V4743 Sagittarii

Astronomy and Astrophysics

Volumn 431, Issue 1, 2005, Pages 321-328

  Petz, A ^a   Hauschildt, P H ^a   Ness, J U ^a   Starrfield, S ^b  

^a UNIVERSITY OF HAMBURG   (Germany)

^b ARIZONA STATE UNIVERSITY   (United States)

Author keywords

Atomic data; Stars: atmospheres; Stars: novae, cataclysmic variables; X rays: individuals: V4743 Sgr

Indexed keywords

CODES (SYMBOLS); CONTINUUM MECHANICS; DATABASE SYSTEMS; EARTH ATMOSPHERE; ENERGY CONSERVATION; MATHEMATICAL MODELS; SATELLITES; SOLAR SYSTEM; SPECTRUM ANALYSIS; THERMODYNAMIC PROPERTIES; X RAYS;

ATOMIC DATA; CATACLYSMIC VARIABLES; STARS: ATMOSPHERES; STARS: NOVAE; V4743 SGR; X-RAYS: INDIVIDUALS;

ASTROPHYSICS;

EID: 13844254265     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041396     Document Type: Article

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