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| Query : 2021MNRAS.505L.112E |
2021MNRAS.505L.112E - Mon. Not. R. Astron. Soc., 505, L112-L114 (2021/July-3)
The minimum rotation period of millisecond pulsars.
ERTAN U. and ALPAR M.A.
Abstract (from CDS):
A simple and natural explanation for the minimum period of millisecond pulsars follows from a correlation between the accretion rate and the frozen surface dipole magnetic field resulting from ohmic diffusion through the neutron star crust in initial stages of accretion in low-mass X-ray binaries.
Abstract Copyright: © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society
Journal keyword(s): stars: neutron - pulsars: general - pulsars: millisecond - binaries: low-mass X-ray
Simbad objects: 3
| Number of rows : 3 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | PSR J1748-2446ad | Psr | 17 48 04.9 | -24 46 04 | ~ | 141 | 1 | |||||
| 2 | SAX J1808.4-3658 | LXB | 18 08 27.58 | -36 58 43.9 | ~ | 1051 | 0 | |||||
| 3 | PSR B1937+21.4 | Psr | 19 39 38.560096 | +21 34 59.13552 | ~ | 1142 | 0 |
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