Neutron stars, strange pulsars and stran
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Fridolin Weber; M.K. Weigel; N.K. Glendenning
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Article
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1997
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Elsevier Science
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English
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This paper deals with an investigation of the properties of hypothetical strange-matter stars, which are composed of u, d, s quark matter whose energy per baryon number lies below the one of ~6Fe. Observable quantities which allow to distinguish such objects from their "conventional" counterparts, i