Search results for " Astrophysics - Solar and Stellar Astrophysics"

showing 2 items of 2 documents

Impulsive coronal heating from large-scale magnetic rearrangements: from IRIS to SDO/AIA

2019

The Interface Region Imaging Spectrograph (IRIS) has observed bright spots at the transition region footpoints associated with heating in the overlying loops, as observed by coronal imagers. Some of these brightenings show significant blueshifts in the Si iv line at 1402.77 A (logT[K] = 4.9). Such blueshifts cannot be reproduced by coronal loop models assuming heating by thermal conduction only, but are consistent with electron beam heating, highlighting for the first time the possible importance of non-thermal electrons in the heating of non-flaring active regions. Here we report on the coronal counterparts of these brightenings observed in the hot channels of the Atmospheric Imaging Assem…

010504 meteorology & atmospheric sciencesSun: activity Sun: corona Sun: UV radiation Astrophysics - Solar and Stellar AstrophysicsFOS: Physical sciencesAstrophysicsElectron01 natural sciences0103 physical sciencesmedicineAstrophysics::Solar and Stellar AstrophysicsIris (anatomy)010303 astronomy & astrophysicsSpectrographSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesLine (formation)PhysicsAstronomy and AstrophysicsCoronal loopThermal conductionmedicine.anatomical_structureAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceCoronal planePhysics::Space PhysicsCathode rayAstrophysics::Earth and Planetary Astrophysics
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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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