Nature, Volume 253 |
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Page 28
These values for energy emission are considerably Smaller than the Eddington
limit and so matter could accrete on to the neutron star. If the radio emission
process is to continue, that matter must absorb the radio radiation by the free-free
...
These values for energy emission are considerably Smaller than the Eddington
limit and so matter could accrete on to the neutron star. If the radio emission
process is to continue, that matter must absorb the radio radiation by the free-free
...
Page 173
Emission at Ho is found to be a more common Phenomenon among the Algol-
type eclipsing binaries than was thought before. Usually, but not always, the
emission is best observed during the primary minimum when the light of the
hotter and ...
Emission at Ho is found to be a more common Phenomenon among the Algol-
type eclipsing binaries than was thought before. Usually, but not always, the
emission is best observed during the primary minimum when the light of the
hotter and ...
Page 250
On the basis of the above considerations, one would expect a bremsstrahlung
spectrum below ~ hop, ; although the shape of the spectrum above - hop, is
difficult to determine, one might expect a steep fall-off because of cyclotron
emission.
On the basis of the above considerations, one would expect a bremsstrahlung
spectrum below ~ hop, ; although the shape of the spectrum above - hop, is
difficult to determine, one might expect a steep fall-off because of cyclotron
emission.
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Bibliographic information
| Title | Nature, Volume 253 Marilee E. Thomas and Robert C. Thomas Science and Related Subjects Collection |
| Editor | Sir Norman Lockyer |
| Publisher | Macmillan Journals Limited, 1975 |
| Original from | the University of Michigan |
| Digitized | 16 Jul 2009 |
| Export Citation | BiBTeX EndNote RefMan |