Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 837
Equation ( 10 ) shows that , starting from mi > mo , mass loss from the primary
results in a decrease of a , until mı = mg . After this , further mass loss from the
primary results in an increase of a . Since , for decreasing mi / m2 , also ry
decreases ...
Equation ( 10 ) shows that , starting from mi > mo , mass loss from the primary
results in a decrease of a , until mı = mg . After this , further mass loss from the
primary results in an increase of a . Since , for decreasing mi / m2 , also ry
decreases ...
Page 838
The variation of the thermal - equilibrium radius of the primary component Rı and
the radius of its Roche lobe r , during the mass transfer from primary to secondary
. Only after the roles of primary and secondary have been reversed will r ...
The variation of the thermal - equilibrium radius of the primary component Rı and
the radius of its Roche lobe r , during the mass transfer from primary to secondary
. Only after the roles of primary and secondary have been reversed will r ...
Page 839
Then , for « low - mass » systems [ 32 , 33 ) , the primary has become an
overluminous subgiant in the shell hydrogen - burning stage ( with a degenerate
helium core ) . The envelope continues to expand on a nuclear time scale and
slow ...
Then , for « low - mass » systems [ 32 , 33 ) , the primary has become an
overluminous subgiant in the shell hydrogen - burning stage ( with a degenerate
helium core ) . The envelope continues to expand on a nuclear time scale and
slow ...
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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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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.", Societą italiana di fisica Rivista del nuovo cimento |
| Contributor | Societą 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 |