English
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About The Book
Description
Author
This text describes the microscopic physics operating in stars and demonstrates how stars respond from formation through hydrogen-burning phases up to the onset of helium burning. The volume contains many illustrations and detailed numerical solutions to prepare beginning graduate students and senior undergraduates to program and calculate evolutionary models.
Piracy-free
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Details
ISBN 13
9781107016569
Publication Date
-29-11-2012
Pages
-908
Weight
-1676 grams
Dimensions
-177.8x254x48.65 mm
