Table 1:
Known and likely DNS binaries. Listed are the pulse period ![]() ![]() ![]() ![]() ![]() ![]() |
Table 2:
Parameters for the 20 isolated millisecond pulsars currently known in the Galactic disk. Four of the pulsars (J0609+2130, J1038+0032, J1753–1914 and J2235+1506) are thought to be the descendants of high-mass binary systems. Listed are the spin period ![]() ![]() ![]() ![]() ![]() ![]() |
Table 3:
Parameters for the 19 eccentric (e > 0.05) binary pulsars currently known that are not in globular clusters. In addition to the parameters listed in Table 2, we also give the binary period ![]() ![]() ![]() ![]() ![]() |
Table 4:
Parameters for 64 low-eccentricity binary pulsars currently known in the Galactic disk. The parameters listed are defined in Tables 2 and 3. |
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