The Distribution of Ages, Magnetic Fields and Spin Periods of Millisecond Pulsars

Details The Distribution of Ages, Magnetic Fields and Spin Periods of Millisecond Pulsars The Distribution of Ages, Magnetic Fields and Spin Periods of Millisecond Pulsars

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...20911505k&link_type=abstract

2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #115.05; Bulletin of the American Astronomical Society,

Astronomy and Astrophysics

Astronomy

Scientific paper

The origin of the bimodal magnetic field distribution of Millisecond Pulsars (MSPs) has been a subject of debate for more than 14 yrs. We show that the effect of secular acceleration to the observed spin down rate of some of the nearby PSRs is significant. We will review the latest age and magnetic field distribution of MSPs and discuss the ramifications on the initial spin periods, characteristic ages, evolution and the accretion history of MSPs.

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