Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 38
summarized in several reviews ( GIACCONI [ 37 ] ) and the optical data which
give the measured mass are discussed by BAHCALL in this volume . It is
interesting that the interpretation above has been strengthened rather than
weakened by ...
summarized in several reviews ( GIACCONI [ 37 ] ) and the optical data which
give the measured mass are discussed by BAHCALL in this volume . It is
interesting that the interpretation above has been strengthened rather than
weakened by ...
Page 377
Qualitatively these two cases give the same result : the ignition ... The issue is
further confused by the fact that most standard procedures used in rezoning
stellar evolutionary models give rise to numerical diffusion . Interpolation of zones
in ...
Qualitatively these two cases give the same result : the ignition ... The issue is
further confused by the fact that most standard procedures used in rezoning
stellar evolutionary models give rise to numerical diffusion . Interpolation of zones
in ...
Page 486
In table I of their paper , the authors give five sets of the coefficients Cn and n ,
that enter in the definition of the new potential ( x = 0 . 7r ) exp [ - Na ] + V ( r ) . (
36 ) Visj ( r ) = EC , n1 The coefficient C , and the tensor V , are taken from the
one ...
In table I of their paper , the authors give five sets of the coefficients Cn and n ,
that enter in the definition of the new potential ( x = 0 . 7r ) exp [ - Na ] + V ( r ) . (
36 ) Visj ( r ) = EC , n1 The coefficient C , and the tensor V , are taken from the
one ...
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Contents
Gruppo fotografico del partecipanti al Corso | 1 |
Introduction | 17 |
Сen | 37 |
Copyright | |
59 other sections not shown
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Common terms and phrases
absorption accretion amplitude analysis angular approximation assumed Astrophys binary black hole calculations charge considered convective core corresponding cycle density dependence detailed detectors determined dips discussed disk distance eclipse effect electromagnetic electron emission energy equation estimate evolution existence expected field Figure flux frequency function geometry give given gravitational important increase indicated intensity interesting Journ less Lett light curve limit lines magnetic mass mean measurements motion Nature neutrino neutron star observed obtained occur optical orbital parameters particle period phase Phys position possible potential present primary pulsations radiation radio range ratio region relation relative rotating scale sensitivity shell shown shows solutions spectrum stellar stellar wind structure suggested surface temperature values variable variations velocity X-ray sources
Bibliographic information
| Title | Proceedings of the International School of Physics "Enrico Fermi.", Volume 65 Proceedings of the International School of Physics "Enrico Fermi.", Società italiana di fisica Rivista del nuovo cimento |
| Contributor | Società italiana di fisica |
| Publisher | N. Zanichelli, 1978 |
| Original from | the University of California |
| Digitized | 14 Aug 2008 |
| ISBN | 0720407206, 9780720407204 |
| Export Citation | BiBTeX EndNote RefMan |