Minimum Accretion Rate for Millisecond Pulsar Formation in Binary System
classification
🌌 astro-ph.HE
keywords
accretionmillisecondpulsarratebinaryminimumformationpulsars
pith:3NTUJD6F Add to your LaTeX paper
What is a Pith Number?\usepackage{pith}
\pithnumber{3NTUJD6F}
Prints a linked pith:3NTUJD6F badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more
read the original abstract
186 binary pulsars are shown in the magnetic field versus spin period (B-P) dia- gram, and their relations to the millisecond pulsars can be clearly seen. We declaim a minimum accretion rate for the millisecond pulsar formation both from the observation and theory. If the accretion rate is lower than the minimum accretion rate, the pulsar in binary system will not become a millisecond pulsar after the evolution.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.