The nature of millisecond pulsars with helium white dwarf companions
We examine the growing data set of binary millisecond pulsars that are thought to have a helium white dwarf companion. These systems are believed to form when a low- to intermediatemass companion to a neutron star fills its Roche lobe between central hydr
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Smedley_The_nature_of_millisecond_2014.pdf||3 MB||Adobe PDF|
Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.