William Bromwich; Joachim Gschwinder; Gerhard Kronisch; Achim Seifert; Manfred Weiss Nomos Verlagsges.MBH + Co (2010) Saatavuus: Hankintapalvelu Pehmeäkantinen kirja
Holger Weiss; Joachim Mickwitz; Laura Hollsten; Anna Sundelin; Kalle Kananoja; Holger Weiss Bokförlaget Nya Doxa (2010) Saatavuus: Tilaustuote Kovakantinen kirja
Joachim Rautenberg; Peter Fritsch; Winfried Hoch; Gerhard Merkl; Franz Otillinger; Matthias Weiss; Burkhard Wricke Springer Vieweg (2013) Saatavuus: Hankintapalvelu Kovakantinen kirja
Blohm; Ernst Gottlieb Baron; Paul Charles Durant; Bernhard Joachim Hagen; Silvius Leopold Weiss Julkaisija: Hänssler (2021) Saatavuus: Tilaustuote CD-levy
Sven Kuhrau; Isabelle von Marschall; Liliane Weissberg; Joachim Rees; Alexis Joachimides; Ulrike Wolff-Thomsen; Mi Zajonz DruckVerlag Kettler (2010) Saatavuus: Tulossa! Kovakantinen kirja
Wolfgang Bischof; Ulf Köpcke; Joachim Zeller; Torsten Bolender; Armin Weissmüller; Anne Fingerling Fachverband Luftdichtheit (2012) Saatavuus: Tilaustuote Pehmeäkantinen kirja
Springer Sivumäärä: 604 sivua Asu: Kovakantinen kirja Painos: 2 Julkaisuvuosi: 2012, 30.10.2012 (lisätietoa) Kieli: Englanti
This long-awaited second edition of the classical textbook on Stellar Structure and Evolution by Kippenhahn and Weigert is a thoroughly revised version of the original text. Taking into account modern observational constraints as well as additional physical effects such as mass loss and diffusion, Achim Weiss and Rudolf Kippenhahn have succeeded in bringing the book up to the state-of-the-art with respect to both the presentation of stellar physics and the presentation and interpretation of current sophisticated stellar models. The well-received and proven pedagogical approach of the first edition has been retained.
The book provides a comprehensive treatment of the physics of the stellar interior and the underlying fundamental processes and parameters. The models developed to explain the stability, dynamics and evolution of the stars are presented and great care is taken to detail the various stages in a star’s life. Just as the first edition, which remained astandard work for more than 20 years after its first publication, the second edition will be of lasting value not only for students but also for active researchers in astronomy and astrophysics.