Relationship between X-ray and ultraviolet emission of flares from dMe stars observed by XMM-Newton

Autor: A. J. J. Raassen, R. Mewe, L. van Driel-Gesztelyi, Graziella Branduardi-Raymont, Manuel Guedel, Louise K. Harra, H. R. M. Kay, Urmila Mitra-Kraev, Marc Audard
Přispěvatelé: University College of London [London] (UCL), Paul Scherrer Institute, Columbia Astrophysics Laboratory, Columbia University, New York, SRON Netherlands Institute for Space Research, Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Physique solaire, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, High Energy Astrophys. & Astropart. Phys (API, FNWI)
Jazyk: angličtina
Rok vydání: 2005
Předmět:
Zdroj: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2005, 431, pp.679-686. ⟨10.1051/0004-6361:20041201⟩
Astronomy & Astrophysics, 431(2), 679-686. EDP Sciences
ISSN: 0004-6361
DOI: 10.1051/0004-6361:20041201⟩
Popis: We present simultaneous ultraviolet and X-ray observations of the dMe-type flaring stars AT Mic, AU Mic, EV Lac, UV Cet and YZ CMi obtained with the XMM-Newton observatory. During 40 hours of simultaneous observation we identify 13 flares which occurred in both wave bands. For the first time, a correlation between X-ray and ultraviolet flux for stellar flares has been observed. We find power-law relationships between these two wavelength bands for the flare luminosity increase, as well as for flare energies, with power-law exponents between 1 and 2. We also observe a correlation between the ultraviolet flare energy and the X-ray luminosity increase, which is in agreement with the Neupert effect and demonstrates that chromospheric evaporation is taking place.
Comment: 8 pages, 4 figures, 3 tables, accepted by A&A (30 Sept. 2004)
Databáze: OpenAIRE