Search results for "abundances"

showing 3 items of 43 documents

The Gaia-ESO Survey: impact of extra mixing on C and N abundances of giant stars

2018

The GES survey using FLAMES at the VLT has obtained high-resolution UVES spectra for a large number of giant stars, allowing a determination of the abundances of the key chemical elements C and N at their surface. The surface abundances of these chemical species are well-known to change in stars during their evolution on the red giant branch after the first dredge-up episod, as a result of extra-mixing phenomena. We investigate the effects of thermohaline mixing on C and N abundances using the first comparison between the GES [C/N] determinations with simulations of the observed fields using a model of stellar population synthesis. We explore the effects of thermohaline mixing on the chemic…

stars: abundances010504 meteorology & atmospheric sciencesStellar populationMetallicityFOS: Physical sciencesabundances ; stars: evolution ; galaxy: stellar content ; galaxy: abundances ; astrophysics - solar and stellar astrophysics [stars]AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAstronomi astrofysik och kosmologi0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicsstellar content [Galaxy]Astronomy Astrophysics and Cosmologystars: evolution14. Life underwater010303 astronomy & astrophysicsStellar evolutionSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsGalaxy: stellar contentabundances [Galaxy]Astronomy and AstrophysicsGiant starRed-giant branchabundances [stars]StarsAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceGlobular clusterevolution [stars]Galaxy: abundancesAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Open cluster
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X-ray emission from the old CTTS MP Muscae

2007

We study the properties of X-ray emitting plasma of MP Mus, an old classical T Tauri star. XMM-Newton/RGS spectra allow us to measure the plasma electron density, which probes whether X-ray emission is produced in the accretion process. X-ray emission from MP Mus originates from high density cool plasma but a hot flaring component is also present, suggesting that both coronal magnetic activity and accretion contribute to the observed X-ray emission. From the soft part of the X-ray emission from MP Mus, mostly produced by plasma heated in the accretion shock, we derive the accretion parameters and the characteristics of the shock-heated plasma.

stars: coronaestars: individual: MP MuscaeSettore FIS/05 - Astronomia E Astrofisicastars: abundancesX-rays: starsstars: circumstellar matterstars: pre-main sequence
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X-ray emission from an adolescent classical T Tauri star

2007

stars: coronaestars: individual: MP MuscaeSettore FIS/05 - Astronomia E Astrofisicastars: abundancesX-rays: starsstars: circumstellar matterstars: pre-main sequence
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