Search results for "Stars: flares"

showing 2 items of 2 documents

A coronal explosion on the flare star CN Leonis

2008

We present simultaneous high-temporal and high-spectral resolution observations at optical and soft X-ray wavelengths of the nearby flare star CN Leo. During our observing campaign a major flare occurred, raising the star's instantaneous energy output by almost three orders of magnitude. The flare shows the often observed impulsive behavior, with a rapid rise and slow decay in the optical and a broad soft X-ray maximum about 200 seconds after the optical flare peak. However, in addition to this usually encountered flare phenomenology we find an extremely short (~2 sec) soft X-ray peak, which is very likely of thermal, rather than non-thermal nature and temporally coincides with the optical …

010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics01 natural scienceslaw.inventionSettore FIS/05 - Astronomia E Astrofisicalaw0103 physical sciencesThermalCoronal heatingAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsAstrophysics (astro-ph)Flare starX-rays: stars stars: individual: CN Leo stars: flares stars: coronae stars: activityAstronomy and AstrophysicsX-rays; individual; CN Leo; flares; coronae; stars; activityInstantaneous energyWavelengthSpace and Planetary ScienceRapid riseCoronal planePhysics::Space PhysicsFlare
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Flare diagnostics from loop modeling of a stellar flare observed with XMM-Newton

2006

Abstract XMM-Newton data of an X-ray flare observed on Proxima Centauri provide detailed and challenging constraints for flare modeling. The comparison of the data with the results of time-dependent hydrodynamic loop modeling of this flare allows us to constrain not only the loop morphology, but also the details of the heating function. The results show that even a complex flare event like this can be described with a relatively few – though constrained – components: two loop systems, i.e., a single loop and an arcade, and two heat components, an intense pulse probably located at the loop footpoints followed by a low gradual decay distributed in the coronal part of the loop. The similarity …

PhysicsAtmospheric ScienceSolar flareStars: X-raysAstrophysics::High Energy Astrophysical PhenomenaFlare starAerospace EngineeringAstronomyAstronomy and AstrophysicsAstrophysicsPulse (physics)law.inventionStars: flaresLoop (topology)GeophysicsSpace and Planetary SciencelawPhysics::Space PhysicsAstrophysics::Solar and Stellar AstrophysicsGeneral Earth and Planetary SciencesStars: coronaeLoop modelingSingle loopEvent (particle physics)Flare
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