The origin of peculiar molecular bands in cool DQ white dwarfs

Astronomy and Astrophysics

Volumn 519, Issue 10, 2010, Pages

  Kowalski, P M ^a  

^a GFZ GERMAN RESEARCH CENTRE FOR GEOSCIENCES   (Germany)

Author keywords

Atomic processes; Dense matter; Stars: atmospheres; White dwarfs

Indexed keywords

A-DENSITY; ATOMIC PROCESS; BLUE SHIFT; COOL STARS; CURRENT MODELS; DENSE MATTER; EFFECTIVE TEMPERATURE; ELECTRONIC TRANSITION ENERGIES; HELIUM ATOM; HELIUM DENSITY; IN-LINE; INCOMPLETE KNOWLEDGE; MOLECULAR BAND; MOLECULAR CARBONS; OPTICAL PARTS; ORDER OF MAGNITUDE; PHYSICAL CONDITIONS; QUANTUM MECHANICAL; SHORTER WAVELENGTH; SPECTRAL FEATURE; SPECTROSCOPIC PROPERTY; STARS: ATMOSPHERES; STRONG INTERACTION; SWAN BAND; VIBRATIONAL FREQUENCIES; WHITE DWARFS;

ATOMS; DENSITY FUNCTIONAL THEORY; FLUIDS; HELIUM; QUANTUM THEORY; RADIOACTIVITY;

STARS;

EID: 77956938930     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015238     Document Type: Article

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