A self-consistent model of isolated neutron stars: the case of the X-ray pulsar RX J0720.4-3125

Publisher: Edp Sciences

E-ISSN: 1432-0746|459|1|175-185

ISSN: 0004-6361

Source: Astronomy & Astrophysics, Vol.459, Iss.1, 2006-11, pp. : 175-185

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