Extremely Large Telescopes and the Extremely Small Sources
J.O. Urama^1
1 Dept. of Physics & Astronomy, University of Nigeria, Nsukka
Neutron stars containing typically 1.4 solar masses within a diameter of about 15km are among the smallest astronomical sources and are the densest known form of directly observable matter in the Universe. Many aspects of the neutron star remain poorly understood. Most of the theoretical models on the neutron star, so far, cannot account for many of the observations, which have been largely made at radio wavelengths. This paper discusses the importance of multiwavelength studies, using large telescopes, to better understand the properties and behaviour of these objects.

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On 20 Oct 2005, 17:41.