UID:
edocfu_9959238883902883
Format:
1 online resource (x, pages 893-1495) :
,
digital, PDF file(s).
ISBN:
1-316-08960-6
,
1-139-77956-7
,
1-139-77652-5
,
1-139-06123-2
,
1-139-78352-1
,
1-139-78255-X
Series Statement:
Stellar evolution physics ; v. 2
Content:
This volume explains the microscopic physics operating in stars in advanced stages of their evolution and describes with many numerical examples and illustrations how they respond to this microphysics. Models of low and intermediate mass are evolved through the core helium-burning phase, the asymptotic giant branch phase (alternating shell hydrogen and helium burning) and through the final cooling white dwarf phase. A massive model is carried from the core helium-burning phase through core and shell carbon-burning phases. Gravothermal responses to nuclear reaction-induced transformations and energy loss from the surface are described in detail. Written for senior graduate students and researchers who have mastered the principles of stellar evolution, as developed in the first volume of Stellar Evolution Physics, sufficient attention is paid to how numerical solutions are obtained to enable the reader to engage in model construction on a professional level.
Note:
Title from publisher's bibliographic system (viewed on 05 Oct 2015).
,
-- pt. IV. Transport processes, weak interaction processes, and helium-burning reactions -- pt. V. Evolution during helium-burning phases -- pt. VI. Terminal evolution of low and intermediate mass stars.
,
English
Additional Edition:
ISBN 1-107-01657-6
Language:
English
