Search results for "stars : late-type"

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X-ray spectral and timing characteristics of the stars in the young open cluster IC 2391

2005

We present X-ray spectral and timing analysis of members of the young open cluster IC 2391 observed with the XMM-Newton observatory. We detected 99 X-ray sources by analysing the summed data obtained from MOS1, MOS2 and pn detectors of the EPIC camera; 24 of them are members, or probable members, of the cluster. Stars of all spectral types have been detected, from the early-types to the late-M dwarfs. Despite the capability of the instrument to recognize up to 3 thermal components, the X-ray spectra of the G, K and M members of the cluster are well described with two thermal components (at kT$_1 \sim$ 0.3-0.5 keV and kT$_2 \sim$ 1.0-1.2 keV respectively) while the X-ray spectra of F members…

Physicsopen clusters and associations : individual : IC 2391 OPEN CLUSTERSAstrophysics (astro-ph)X-rayFOS: Physical sciencesstars : late-typeAstronomy and AstrophysicsAstrophysicsX-ray : starAstrophysicsStellar classificationSpectral linePLEIADESstars : activityVARIABILITYStarsSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceObservatoryROSATstars; stars : activity; stars : early-type; stars : late-type; open clusters and associations : individual : IC 2391 OPEN CLUSTERS; EMISSION; PLEIADES; VARIABILITY [X-ray]Cluster (physics)stars : early-typeEMISSIONOpen clusterAstronomy & Astrophysics
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Spectral properties of X-ray bright variable sources in the Taurus Molecular Cloud

2006

We analyze 19 bright variable X-ray sources detected in the XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST), in order to characterize the variations with time of their coronal properties and to derive informations on the X-ray emitting structures. We performed time-resolved spectroscopy of the EPIC PN and MOS spectra of the XEST sources, using a model with one or two thermal components, and we used the time evolution of the temperatures and emission measures during the decay phase of flares to derive the size of the flaring loops. The light curves of the selected sources show different types of variability: flares, long-lasting decay or rise through the whole observation, sl…

stars : pre-main sequence010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaX-rays : starsFOS: Physical sciencesFluxAstrophysicsAstrophysics01 natural sciences7. Clean energySpectral linelaw.inventionlaw0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsSpectroscopy010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsMolecular cloudAstrophysics (astro-ph)Astronomy and Astrophysicsstars : late-typeRadiusPlasmaLight curve13. Climate actionSpace and Planetary Sciencestars : coronaeFlare
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