Consequences of a strong phase transition in the dense matter equation of state for the rotational evolution of neutron stars

Author: Bejger M.   Blaschke D.   Haensel P.   Zdunik J. L.   Fortin M.  

Publisher: Edp Sciences

E-ISSN: 1432-0746|600|issue|A39-A39

ISSN: 0004-6361

Source: Astronomy & Astrophysics, Vol.600, Iss.issue, 2017-03, pp. : A39-A39

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Abstract