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A&A 416, 733747 (2004) DOI: 10.1051/0004-6361:20034027
 

Summary: A&A 416, 733­747 (2004)
DOI: 10.1051/0004-6361:20034027
c ESO 2004
Astronomy
&
Astrophysics
Modeling an X-ray flare on Proxima Centauri: Evidence
of two flaring loop components and of two heating
mechanisms at work
F. Reale1, M. G¨udel2, G. Peres1, and M. Audard3
1
Dipartimento di Scienze Fisiche & Astronomiche, Sezione di Astronomia, Universit`a di Palermo, Piazza del Parlamento 1,
90134 Palermo, Italy
e-mail: peres@astropa.unipa.it
2
Paul Scherrer Institut, W¨urenlingen & Villigen, 5232 Villigen PSI, Switzerland
e-mail: guedel@astro.phys.ethz.ch
3
Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY 10027, USA
e-mail: audard@astro.columbia.edu

  

Source: Audard, Marc - INTEGRAL Science Data Centre & Observatory of Geneva, Université de Genève

 

Collections: Physics