Publication Abstracts

Finzi and Wolf 1968

Finzi, A., and R.A. Wolf, 1968: Hot, vibrating neutron stars. Astrophys. J., 153, 835-848, doi:10.1086/149708.

Taking into account the dissipative effect of neutrino-producing reactions, we calculate the amount of thermal and vibrational energy that can be present in a neutron star at a tiine t after its creation in a supernova explosion.

The results are used to discuss the plausibility of a number of hypotheses advanced in recent years concerning possible observable properties of neutron stars.

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BibTeX Citation

  author={Finzi, A. and Wolf, R. A.},
  title={Hot, vibrating neutron stars},
  journal={Astrophys. J.},

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RIS Citation

ID  - fi09000a
AU  - Finzi, A.
AU  - Wolf, R. A.
PY  - 1968
TI  - Hot, vibrating neutron stars
JA  - Astrophys. J.
VL  - 153
SP  - 835
EP  - 848
DO  - 10.1086/149708
ER  -

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