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Deriving fundamental parameters of millisecond pulsars via AIC in white dwarfs

Published online by Cambridge University Press:  21 February 2013

A. Taani ,
C. M. Zhang ,
Y. H. Zhao  and
A. Moraghan
A. Taani*
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
C. M. Zhang
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
Y. H. Zhao
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
A. Moraghan
Affiliation:
Center for Galaxy Evolution Research and Department of Astronomy, Yonsei University, Seoul 120-749, Republic of Korea
*
†email: alitaani@bao.ac.cn
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Abstract

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We present a study of the observational properties of Millisecond Pulsars (MSPs) by way of their magnetic fields, spin periods and masses. These measurements are derived through the scenario of Accretion Induced Collapse (AIC) of white dwarfs (WDs) in stellar binary systems, in order to provide a greater understanding of the characteristics of MSP populations. In addition, we demonstrate a strong evolutionary connection between neutron stars and WDs with binary companions from a stellar binary evolution perspective via the AIC process.

Keywords

Neutron starswhite dwarfscataclysmic variablesfundamental parameters
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S290: Feeding Compact Objects: Accretion on All Scales , August 2012 , pp. 177 - 178
Copyright
Copyright © International Astronomical Union 2013

References

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