Search results for "radiative transfer — stars: coronae — stars: late-type — X-rays: stars"

showing 1 items of 1 documents

On X-ray Optical Depth in the Coronae of Active Stars

2007

We have investigated the optical thickness of the coronal plasma through the analysis of high-resolution X-ray spectra of a large sample of active stars observed with the High Energy Transmission Grating Spectrometer on Chandra. In particular, we probed for the presence of significant resonant scattering in the strong Lyman series lines arising from hydrogen-like oxygen and neon ions. The active RS CVn-type binaries II Peg and IM Peg and the single M dwarf EV Lac show significant optical depth. For these active coronae, the Lya/Lyb ratios are significantly depleted as compared with theoretical predictions and with the same ratios observed in similar active stars. Interpreting these decremen…

PhysicsLyman seriesAstrophysics (astro-ph)chemistry.chemical_elementFluxFOS: Physical sciencesAstronomy and AstrophysicsRadiusAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsradiative transfer — stars: coronae — stars: late-type — X-rays: starsSpectral linesymbols.namesakeStarsNeonchemistrySpace and Planetary SciencesymbolsAstrophysics::Solar and Stellar AstrophysicsOptical depthLine (formation)
researchProduct