Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page xviii
821 E . P . J . VAN DEN HEUVEL – Evolution of close binaries , with possible
applications to massive X - ray binaries . » 828 » > > » 831 831 831 833 833 834
834 835 » » 1 . Introduction . . . . . . . . . . . . . . . . . . . . 2 . Evolution of single stars ...
821 E . P . J . VAN DEN HEUVEL – Evolution of close binaries , with possible
applications to massive X - ray binaries . » 828 » > > » 831 831 831 833 833 834
834 835 » » 1 . Introduction . . . . . . . . . . . . . . . . . . . . 2 . Evolution of single stars ...
Page 356
The Final Stages of the Evolution of Single Stars . W . D . ARNETT ( * )
Department of Astronomy , University of Illinois - Urbana , III . 61801 Introduction .
In these lectures I will survey the late ( and perhaps final ) stages of evolution of
stars ...
The Final Stages of the Evolution of Single Stars . W . D . ARNETT ( * )
Department of Astronomy , University of Illinois - Urbana , III . 61801 Introduction .
In these lectures I will survey the late ( and perhaps final ) stages of evolution of
stars ...
Page 398
the evolution was rapid would appear expanded . The main features of the
evolution are as follows . The temperature rises rapidly until the edge of the
convective region approaches densities at which decay of 23Ne can occur on a
reasonable ...
the evolution was rapid would appear expanded . The main features of the
evolution are as follows . The temperature rises rapidly until the edge of the
convective region approaches densities at which decay of 23Ne can occur on a
reasonable ...
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Contents
Gruppo fotografico del partecipanti al Corso | 1 |
Introduction | 17 |
Сen | 37 |
Copyright | |
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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