Dim isolated neutron stars, cooling and energy dissipation

ISSN： 0004-640X

Source： Astrophysics and Space Science, Vol.308, Iss.1-4, 2007-04, pp. : 133-136

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content

Accretion by isolated neutron stars

By Ikhsanov N.

Astrophysics and Space Science, Vol. 308, Iss. 1-4, 2007-04 ,pp. : 137-140

Springer Publishing Company

Access to resources Recommend Favorite

Cooling of neutron stars with strong toroidal magnetic fields

By Page Dany

Astrophysics and Space Science, Vol. 308, Iss. 1-4, 2007-04 ,pp. : 403-412

Springer Publishing Company

Access to resources Recommend Favorite

Cooling rates of neutron stars and the young neutron star in the Cassiopeia A supernova remnant

By Yakovlev Dmitry G. Ho Wynn C. G. Shternin Peter S. Heinke Craig O. Potekhin Alexander Y.

Monthly Notices of the Royal Astronomical Society, Vol. 411, Iss. 3, 2011-03 ,pp. : 1977-1988

Oxford University Press

Access to resources Recommend Favorite

Symmetry of the neutron and proton superfluidity effects in cooling neutron stars

By Gusakov M. Kaminker A. Yakovlev D. Gnedin O.

Astronomy Letters, Vol. 30, Iss. 11, 2004-11 ,pp. : 759-771

MAIK Nauka/Interperiodica

Access to resources Recommend Favorite

Cooling of neutron stars: Two types of triplet neutron superfluidity

By Gusakov M. Gnedin O.

Astronomy Letters, Vol. 28, Iss. 10, 2002-10 ,pp. : 669-675

MAIK Nauka/Interperiodica

Access to resources Recommend Favorite