Massive Stars and their Supernovae
by F. Thielemann, R. Hirschi, M. Liebendorfer, R. Diehl
Publisher: arXiv 2010
Number of pages: 81
Description:
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).
Download or read it online for free here:
Download link
(5.6MB, PDF)
Similar books
A Practical Introduction to Numerical Hydrodynamics
by Garrelt Mellema - Leiden University
An introduction to the field of numerical hydrodynamics. It will give you some insight in what is involved in such calculations. Numerical hydrodynamics is used in many parts of astrophysics. The applications we consider in this exercise are stellar.
(9909 views)
by Garrelt Mellema - Leiden University
An introduction to the field of numerical hydrodynamics. It will give you some insight in what is involved in such calculations. Numerical hydrodynamics is used in many parts of astrophysics. The applications we consider in this exercise are stellar.
(9909 views)
Images of the Solar Upper Atmosphere From SUMER on SOHO
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.
(6586 views)
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.
(6586 views)
An Introduction to the Theory of Rotating Relativistic Stars
by Eric Gourgoulhon - arXiv
These notes introduce the theory of rotating stars in general relativity. The focus is on the theoretical foundations, with a detailed discussion of the spacetime symmetries, the choice of coordinates and the derivation of the equations of structure.
(6633 views)
by Eric Gourgoulhon - arXiv
These notes introduce the theory of rotating stars in general relativity. The focus is on the theoretical foundations, with a detailed discussion of the spacetime symmetries, the choice of coordinates and the derivation of the equations of structure.
(6633 views)
Supernovae
- Wikipedia
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.
(3213 views)
- Wikipedia
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.
(3213 views)