by J. B. Tatum
A course on stellar atmospheres which covers: definitions of and relations between quantities used in radiation theory, blackbody radiation, the exponential integral function, flux, specific intensity and other astrophysical terms, absorption, scattering, extinction and the equation of transfer, limb darkening, atomic spectroscopy, Boltzmann's and Saha's equations, oscillator strengths and related topics, line profiles, curve of growth.
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by Simon C. O. Glover - arXiv
The author discusses our current understanding of the physical processes involved in the formation of Population III stars. He shows how we can identify the mass scale of the first dark matter halos to host Population III star formation.
by Andreas Schmitt - arXiv
Cold and dense nuclear and quark matter can be found in the interior of compact stars. The author gives a pedagogical introduction to microscopic calculations based on phenomenological models, effective theories, and perturbative QCD.
by Uri Feldman, at al. - ESA Publications Division
Investigations of the heating of the corona and the acceleration of the solar wind are two of the prime scientific goals in studying the solar upper atmosphere with the Solar and Heliospheric Observatory (SOHO) of ESA and NASA.
by Gerard 't Hooft - Utrecht University
Contents: The Metric of Space and Time; Curved coordinates; A short introduction to General Relativity; Gravity; The Schwarzschild Solution; The Chandrasekhar Limit; Gravitational Collapse; The Reissner-Nordstrom Solution; Horizons; and more.