Titlebook: Hot Thin Plasmas in Astrophysics; Roberto Pallavicini (Director of the ASI) Book 1988 Kluwer Academic Publishers 1988 Galaxy.LOPES.Librati

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Diagnostic Techniques for Hot Thin Astrophysical Plasmas multiply ionized atoms and for their interpretation in terms of physical parameters it is necessary to understand the atomic processes involved and to compute the corresponding parameters. These X-ray diagnostic techniques are used mainly for solar active regions and flare plasmas. Spectra from Ca

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Instrumentation for the Study of Cosmic X-Ray Plasmasnent features of X-ray missions now being developed. X-ray concentrators, energy sensitive broad-band imaging detectors and wavelength dispersive gratings and crystals can be combined to provide powerful tools for performing diagnostic measurements on cosmic X-ray plasmas. A selection of these devic

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BURSA

Constrain

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Re-Analysis of the Coronal Emission from RS CVn Type Binariesexplore the activity parameters in these systems. It is well established that the x-ray luminosity L. is correlated with the Roche lobe filling percentage RL and the radius R where I belive, RL and R represent the depth I of the sub-photospheric convective layer. It is known that I is the basic para

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High Resolution Soft X-Ray Spectroscopy of Hot White Dwarfsr on EXOSAT. These data, which are unique in wavelength coverage, spectral resolution, and statistical quality, have offered us the first detailed look at the photospheric X-ray spectrum of these objects. The shape of the soft X-ray spectrum is highly sensitive to the spectral parameters; we use thi

CHYME

Pulsating White Dwarfs. Pulsational instabilities, which arise in three distinct regions along the white dwarf cooling sequence, have periods ranging from 200s to 2500s and offer unique opportunities for the study of the interior and thermal evolution of compact objects. These instabilities are interpreted as non-radial