EPJ Web of Conferences
Volume 7, 2010DM2008 – Dense Matter in Heavy-Ion Collisions and Astrophysics
|Number of page(s)||62|
|Published online||05 October 2010|
Isolated Neutron Stars
Sternberg Astronomical Institute, Moscow, Russia
Several aspects related to astrophysics of isolated neutron stars are discussed. We start with an introduction into the “new zoo” of young isolated neutron stars. In addition to classical radio pulsars, now we know several species (soft gamma-ray repeators, anomalous X-ray pulsars, central compact objects in supernova remnants, close-by cooling neutron stars - aka “Magniﬁcent seven”, - RRATs, and some others). All these types are brieﬂy discussed. In the second lecture a description of magneto-rotational evolution of neutron stars is given. Finally, in the third lecture we discuss population synthesis of isolated neutron stars. In some details we discuss population synthesis of young isolated radio pulsars and young close-by cooling neutron stars.
© Owned by the authors, published by EDP Sciences, 2010
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