Search results for "Protoplanetary disk"

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Time Resolved X-Ray Spectral Analysis of Class II YSOs in NGC 2264 During Optical Dips and Bursts

2016

Pre-Main Sequence stars are variable sources. The main mechanisms responsible for their variability are variable extinction, unsteady accretion, and rotational modulation of both hot and dark photospheric spots and X-ray active regions. In stars with disks this variability is thus related to the morphology of the inner circumstellar region (<0.1 AU) and that of photosphere and corona, all impossible to be spatially resolved with present day techniques. This has been the main motivations of the Coordinated Synoptic Investigation of NGC2264, a set of simultaneous observations of NGC2264 with 15 different telescopes. We analyze the X-ray spectral properties of stars with disks extracted du…

Settore FIS/05 - Astronomia E AstrofisicaAccretion accretion disks Stars: pre-main sequence Stars: variables: T Tauri Herbig Ae/BeAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Solar and Stellar Astrophysicspre-main sequence stars; variability protoplanetary disks; accretionAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics::Galaxy Astrophysics
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