Secondary Components of Binary Pulsars & Magnetic Field Decay in Neutron Stars
1987 ◽
Vol 125
◽
pp. 407-407
Keyword(s):
We report the discovery of white dwarf secondaries in 0655+64 and 0820+02 systems. In the 2303+46 system, we do not find any optical counterpart suggesting that the companion is another neutron star. The existence of a cool and therefore old white dwarf in the 0655+64 system implies that the surface magnetic field of neutron stars stops decaying beyond some value(s) of field strength.
1992 ◽
Vol 128
◽
pp. 26-34
Keyword(s):
2010 ◽
Vol 6
(S275)
◽
pp. 309-310
Keyword(s):
2012 ◽
Vol 8
(S291)
◽
pp. 425-427
Keyword(s):
2012 ◽
Vol 8
(S291)
◽
pp. 408-410
Keyword(s):