Search results for "Active star"

showing 3 items of 3 documents

Coronal properties of G-type stars in different evolutionary phases

2005

We report on the analysis of XMM-Newton observations of three G-type stars in very different evolutionary phases: the weak-lined T Tauri star HD 283572, the Zero Age Main Sequence star EK Dra and the Hertzsprung-gap giant star 31 Com. They all have high X-ray luminosity (10^31 erg/s for HD 283572 and 31 Com and 10^30 erg/s for EK Dra). We compare the Emission Measure Distributions (EMDs) of these active coronal sources, derived from high-resolution XMM-Newton grating spectra, as well as the pattern of elemental abundances vs. First Ionization Potential (FIP). We also perform time-resolved spectroscopy of a flare detected by XMM from EK Dra. We interpret the observed $EMD$s as the result of …

G-type main-sequence starLINED T TAURIMetallicityAstrophysics::High Energy Astrophysical PhenomenaX-RAY SPECTROSCOPYFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsLuminosityEMISSION MEASURE DISTRIBUTIONSAstrophysics::Solar and Stellar AstrophysicsACTIVE STARSAstrophysics::Galaxy AstrophysicsXMM-NEWTONPhysicsSOLAR-TYPE STARSAstrophysics (astro-ph)HERTZSPRUNG-GAPAstronomy and AstrophysicsGiant starSurface gravityStarsT Tauri starSpace and Planetary ScienceANALOG EK DRACONISSTELLAR SURFACE-STRUCTUREMAIN-SEQUENCE STARSMain sequence
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The flaring and quiescent components of the solar corona

2008

The solar corona is a template to understand stellar activity. The Sun is a moderately active star, and its corona differs from active stars: active stellar coronae have a double-peaked EM(T) with the hot peak at 8-20 MK, while the non flaring solar corona has one peak at 1-2 MK. We study the average contribution of flares to the solar EM(T) to investigate indirectly the hypothesis that the hot peak of the EM(T) of active stellar coronae is due to a large number of unresolved solar-like flares, and to infer properties on the flare distribution from nano- to macro-flares. We measure the disk-integrated time-averaged emission measure, EM_F(T), of an unbiased sample of solar flares analyzing u…

PhysicsSolar flareAstrophysics (astro-ph)Phase (waves)FOS: Physical sciencesAstronomy and AstrophysicsPlasmaAstrophysicsflaresLight curveAstrophysicsCoronalaw.inventionStarsSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary Sciencelawcoronal heatingcoronaFlareActive star
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Activity, colour anomalies and temperature determination in solar-type stars

2008

PhysicsStarsAstrophysicsType (model theory)Active star
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