Search results for "K-type main-sequence star"

showing 3 items of 23 documents

Signatures of pulsations and mass loss in the spectra of post-AGB stars

2011

AbstractThe results of high-resolution spectroscopy and radial velocity monitoringa are presented for selected post-AGB candidate stars. Time series of high-resolution spectra for HD235858 shows spliting of low-excitation atomic lines and significant changes in the intensity of C2 and CN lines originated in the extended atmosphere significantly affected by pulsations and outflow. Mass ejection was confirmed for cool R CrB candidate stars DY Per, V1983 Cyg, and V2074 Cyg.

PhysicsT Tauri starStarsSpace and Planetary ScienceK-type main-sequence starStellar mass lossAstronomy and AstrophysicsAstrophysicsSpectral lineProceedings of the International Astronomical Union
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Recent X-ray studies of stellar cycles and long-term variability

2006

AbstractWe discuss recent X-ray studies of stellar cycles and long-term variability.

Stars: activityPhysicsStars: magnetic fieldK-type main-sequence starStellar collisionFlare starAstronomyAstronomy and AstrophysicsStars: late-typeAstrophysicsTerm (time)T Tauri starSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceStars: atmosphereStellar mass lossStars: coronaeProceedings of the International Astronomical Union
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Stochastic gravito-inertial modes discovered by CoRoT in the hot Be star HD 51452

2012

International audience; Context. Be stars are rapidly rotating stars with a circumstellar decretion disk. They usually undergo pressure and/or gravity pulsation modes excited by the κ-mechanism, i.e. an effect of the opacity of iron-peak elements in the envelope of the star. In the Milky Way, p-modes are observed in stars that are hotter than or equal to the B3 spectral type, while g-modes are observed at the B2 spectral type and cooler. Aims. We observed a B0IVe star, HD 51452, with the high-precision, high-cadence photometric CoRoT satellite and high-resolution, ground-based HARPS and SOPHIE spectrographs to study its pulsations in great detail. We also used the lower resolution spectra a…

starsBe -stars010504 meteorology & atmospheric sciencesBe starK-type main-sequence staroscillations -starsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsrotation01 natural sciences0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsStellar structureindividual010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciences[PHYS]Physics [physics]PhysicsASTROFÍSICA ESTELARStellar rotationFlare starAstronomyAstronomy and AstrophysicsLight curveESPECTROSCOPIAHD 51452 -starsStarsT Tauri star13. Climate actionSpace and Planetary ScienceAstrophysics::Earth and Planetary Astrophysicsemission-line[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astronomy & Astrophysics
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