Modeling an X-ray flare on Proxima Centauri: Evidence of two flaring loop components and of two heating mechanisms at work

Astronomy and Astrophysics

Volumn 416, Issue 2, 2004, Pages 733-747

  Reale, F ^a   Gudel M ^b   Peres, G ^a   Audard, M ^c  

^a UNIVERSITY OF PALERMO   (Italy)

^b PAUL SCHERRER INSTITUTE   (Switzerland)

^c Och Spine at New York Presbyterian Hospitals   (United States)

Author keywords

Hydrodynamics; Stars: coronae; Stars: flare; X rays: stars

Indexed keywords

COMPUTER SIMULATION; COOLING; HEATING; HYDRODYNAMICS; MORPHOLOGY; PHOTONS; PLASMAS; PROBABILITY; X RAY ANALYSIS;

STARS: CORONAE; STARS: FLARE; X-RAYS: STARS;

ASTROPHYSICS;

EID: 1642285231     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20034027     Document Type: Article

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