The Birth and Death of Stars
by James Schombert
Publisher: University of Oregon 2008
Stars are directly, or indirectly, the source of all the energy necessary to sustain life on our world. This course will study the birth, evolution and death of stars in the Milky Way galaxy, with a particular emphasis on the underlying science behind stellar and galactic evolution, the observational aspect to astronomy and our knowledge of how the Universe operates on the stellar scale.
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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 George W. Collins, II - W H Freeman & Co
The book on stellar astrophysics for the first year graduates or the advanced undergraduate students. It is assumed that the readers have factual knowledge of stars and astronomy. The text describes the axiomatic theory of stellar structure.
A supernova is a stellar explosion that briefly outshines an entire galaxy, radiating as much energy as the Sun or any ordinary star is expected to emit over its entire life span, before fading from view over several weeks or months.
by F. Thielemann, R. Hirschi, M. Liebendorfer, R. Diehl - arXiv
The authors focus on the astrophysical aspects, i.e. a description of the evolution of massive stars and their endpoints, with a special emphasis on the composition of their ejecta in form of stellar winds during the evolution or of explosive ejecta.