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20 April 2024
 
  » arxiv » astro-ph/9911207

 Article overview


The Bologna submillisecond pulsar survey
N. D’Amico ;
Date 11 Nov 1999
Subject astro-ph
AbstractSince the discovery of the original millisecond pulsar, no pulsars with a shorter spin period (P<1.56 ms) were found. However, according to the most popular equations of state, the theoretical limiting spin period of a neutron star can be much shorter. On the other hand, most of the large scale searches for millisecond pulsars carried out so far were strongly biased against the detection of ultrashort periodicities. In this paper we describe a new large scale pulsar survey with a minimum detectable period much shorter than previous searches.
Source arXiv, astro-ph/9911207
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