Bhattacharya, D and Srinivasan, G (1986) On the implication of the recently discovered 5 millisecond binary pulsar PSR 1855+09. In: Current science, 55 (7). 327 -330.
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e argue that the extraordinary fact that all three known millisecond pulsars are very close to the galactic plane implies that there must be ~100 potentially observable millisecond pulsars within ~4 kpc from the Sun. Our other main conclusion is that the dipole magnetic fields or old neutron stars probably saturate around 5 x 108 gauss.
|Item Type:||Journal Article|
|Additional Information:||Copyright of this article belongs to Current science assn.|
|Department/Centre:||Division of Physical & Mathematical Sciences > Physics|
|Date Deposited:||01 Feb 2010 07:25|
|Last Modified:||19 Sep 2010 05:40|
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