Fine-structure infrared lines from the Cassiopeia A knots

Astronomy and Astrophysics

Volumn 509, Issue 1, 2010, Pages

  Docenko, D ^a,b   Sunyaev, R A ^a,c  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b UNIVERSITY OF LATVIA   (Latvia)

^c Department of Satellite Monitoring Technologies   (Russian Federation)

Author keywords

ISM; ISM Atomic processes; Supernova remnants Infrared

Indexed keywords

ASTRONOMY; CHARGE TRANSFER; FORECASTING; NEON; OXYGEN; PHOTOIONIZATION; PLASMA DIAGNOSTICS; SMELTING; SPECTROSCOPY;

ATOMIC PROCESS; CHARGE EXCHANGE PROCESS; CLOUD DENSITY; ELECTRON CONDUCTIVITY; FAR-INFRARED; FINE STRUCTURES; FLUX RATIO; GALACTIC SUPERNOVA; GENERAL MODEL; INFRARED CONTINUUM; INFRARED LINE; ISM - ISM; MODEL PREDICTION; NEAR INFRARED; OXYGEN LINE; PHYSICAL CONDITIONS; PHYSICAL PARAMETERS; PLASMA PARAMETER; SPECTRAL LINE; SPITZER; SUPERNOVA EXPLOSION; SUPERNOVA REMNANTS; TEMPERATURE MODELS; THEORETICAL MODELS;

MODELS;

EID: 76349118329     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200810366     Document Type: Article

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