On stars, their evolution and their stability.

@article{Chandrasekhar1984OnST,
  title={On stars, their evolution and their stability.},
  author={Subrahmanyan Chandrasekhar},
  journal={Science},
  year={1984},
  volume={226 4674},
  pages={
          497-505
        }
}
The Nobel lecture of Chandrasekhar is printed in which he describes the basic processes that determine the life history of a star with particular emphasis on the roles of stellar mass and radiation pressure. (AIP) 
Manybody aspects of gravity in compact stars
Compact stars such as neutron stars and black holes are gravitationally bound many body systems. We investigate the importance of short and long range part of gravity for such systems. From ourExpand
Stability of extended scalar diquark stars vis-à-vis soliton stars
Motivated by relatively large values of the maximum mass (M = 8.92M⊙) and radius (R = 507 km) obtained for an extended scalar diquark star within the framework of an effective φ4-theory (S K KarnetExpand
Stars: Their structure and evolution
The subject of astrophysics began with the study of the stars. It may be recalled that the positivist philosophers who were so influential in European thinking had asserted that it was in the natureExpand
On the Role of Schwarzschild Interaction in Understanding Strong Interaction and Nuclear Binding Energy
In this paper the authors reviewed the basics of final unification with respect to Schwarzschild interaction and strong interaction. In the earlier published papers the authors suggested that,Expand
A Rigorous Examination of the Chandrasekhar Theory of Stellar Collapse
Some of the results of a rigorous analysis of the Chandrasekhar semiclassical theory of stellar collapse are presented here. They are of two kinds. The first concerns the Chandrasekhar equationExpand
Degeneracy, the virial theorem, and stellar collapse
Formulae for the energies of degenerate non-relativistic and ultra-relativistic Fermi gases play multiple roles in simple arguments related to the collapse of a stellar core to a neutron star. TheseExpand
EQUATION-OF-STATE FOR WHITE DWARF STARS
W HITE dwarfs are a distinct class of stellar objects, that were first encountered in F.W. Bessel’s observation of Sirius in 1836. Bessel examined the wobbling features of the proper motion of SiriusExpand
The Dark Universe
For a few years now, cosmology has a standard model. By this term, we mean a consistent theoretical background which is at the same time simple and broad enough to offer coherent explanations for theExpand
The Mysteries of Fermions
It is conjectured that all known fermions are topological solitons. This could explain the non-observation of bosonic leptons and baryons and provide a physical mechanism for the Pauli exclusionExpand
Radioactive beams and nuclear astrophysics
The use of Radioactive Beams, either at low- or at high-energy, in Nuclear Astrophysics, mainly for studying violent stellar events, is reviewed.
...
1
2
3
4
5
...

References

SHOWING 1-10 OF 16 REFERENCES
Mon. Not. Roy. Astr. Soc
  • Mon. Not. Roy. Astr. Soc
  • 1984
Astrophys.J. Supp
  • Astrophys.J. Supp
  • 1983
The author's investigations on the mathematical theory of black holes, continued over the years 1974-1983, are summarized in his last book The Mathematica/ Theory of Black Holes
  • The author's investigations on the mathematical theory of black holes, continued over the years 1974-1983, are summarized in his last book The Mathematica/ Theory of Black Holes
  • 1983
Edward Arthur Milnc: his part in the development of modern astrophysics,
  • Quuart.J. Roy. Astr. Soc.,
  • 1980
The reader may wish to consult the following additional references: 1. Chandrasekhar, S., 'Edward Arthur Milnc: his part in the development of modern astrophysics
  • Quuart.J. Roy. Astr. Soc
  • 1980
‘ Edward Arthur Milnc : his part in the development of modern astrophysics , ’ Quuart
  • J . Roy . Astr . Soc .
  • 1980
Mon. Not. Roy. Astr. Soc. Phys. Rev. Lett
  • Mon. Not. Roy. Astr. Soc. Phys. Rev. Lett
  • 1979
Comm. Math. Phys. Astrophys.J
  • Comm. Math. Phys. Astrophys.J
  • 1977
For an account of these matters pertaining to the classical ellipsoids see Chandrasekhar, S., Ellipsoidal Figures of Equilibrium
  • For an account of these matters pertaining to the classical ellipsoids see Chandrasekhar, S., Ellipsoidal Figures of Equilibrium
  • 1968
...
1
2
...