Search results for " fisica stellare"

showing 2 items of 2 documents

The Mouse That Roared: A Superflare from the dMe Flare Star EV Lac Detected by Swift and Konus-Wind

2010

We report on a large stellar flare from the nearby dMe flare star EV Lac observed by the Swift and Konus-Wind satellites and the Liverpool Telescope. It is the first large stellar flare from a dMe flare star to result in a Swift trigger based on its hard X-ray intensity. Its peak f_X from 0.3--100 keV of 5.3x10^-8 erg/cm2/s is nearly 7000 times larger than the star's quiescent coronal flux, and the change in magnitude in the white filter is >4.7. This flare also caused a transient increase in EV Lac's bolometric luminosity (L_bol) during the early stages of the flare, with a peak estimated L_X/L_bol ~3.1. We apply flare loop hydrodynamic modeling to the plasma parameter temporal changes …

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsLuminositylaw.inventionSettore FIS/05 - Astronomia E AstrofisicalawIonizationX-raysAstrophysics::Solar and Stellar AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysicsFlare starAstronomy and Astrophysicsastrofisica fisica stellare stars: activity stars: coronae stars: flare stars: individual: EV Lac stars: late-type X-rays: starsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceMagnitude (astronomy)Plasma parameterStellar PhysicAstrophysics::Earth and Planetary AstrophysicsSuperflareFlare
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A detailed study of the rise phase of a long duration X-ray flare in the young star TWA 11B

2010

We analyzed a long duration flare observed in a serendipitous XMM-Newton detection of the M star CD-39 7717B (TWA 11B), member of the young stellar association TW Hya (~ 8 Myr). Only the rise phase (with a duration of ~ 35 ks) and possibly the flare peak were observed. We took advantage of the high count-rate of the X-ray source to carry out a detailed analysis of its spectrum during the whole exposure. After a careful analysis, we interpreted the rise phase as resulting from the ignition of a first group of loops (event A) which triggered a subsequent two-ribbon flare (event B). Event A was analyzed using a single-loop model, while a two-ribbon model was applied for event B. Loop semi-leng…

Young stellar objectAstrophysics::High Energy Astrophysical PhenomenaPhase (waves)FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicslaw.inventionSettore FIS/05 - Astronomia E AstrofisicalawIonizationAstrophysics::Solar and Stellar AstrophysicsEmission spectrumAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)X-rayAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesStarsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)astrofisica fisica stellare flares stars: activity stars: coronae stars: flare stars: individual: CD-39 7717B TWA 11B stars: pre-main sequenceAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaEvent (particle physics)Flare
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