Nature, Volume 253 |
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Page 28
Suppose that the density of matter at a distance r from a neutron star of mass, m, (
~ 1 MG) is p. Then ... This gives p < 107* g cm To, and thus in the case of HerX-1
unless the density is higher than about 10−" g cm To, accretion cannot occur.
Suppose that the density of matter at a distance r from a neutron star of mass, m, (
~ 1 MG) is p. Then ... This gives p < 107* g cm To, and thus in the case of HerX-1
unless the density is higher than about 10−" g cm To, accretion cannot occur.
Page 251
Limits on turbulence and convection during the descent are required so that
variations in the density of the infalling plasma are not smoothed out beyond the
timescale of features observed in the Her X-1 pulse profile (rise time as 50 ms).
Limits on turbulence and convection during the descent are required so that
variations in the density of the infalling plasma are not smoothed out beyond the
timescale of features observed in the Her X-1 pulse profile (rise time as 50 ms).
Page 561
The density decreased abruptly at the ventral boundary of the dentate gyrus and
was reduced in the stratum ... The grain density in most sections was distributed
evenly across the stratum moleculare, but in more posterior sections it was much
...
The density decreased abruptly at the ventral boundary of the dentate gyrus and
was reduced in the stratum ... The grain density in most sections was distributed
evenly across the stratum moleculare, but in more posterior sections it was much
...
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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 |