A publishing partnership

The Rotation Rates of White Dwarfs and Pulsars

and

© 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Mario Livio and J. E. Pringle 1998 ApJ 505 339 DOI 10.1086/306153

0004-637X/505/1/339

Abstract

We examine the question of why the white dwarfs in dwarf nova systems are found to be rotating much more slowly than expected. We propose a model in which the accreted angular momentum is removed during nova outbursts. We find that the efficiency of transport of angular momentum between the white dwarf and the extended nova envelope is rather low. We show that in using the same efficiency for the core-envelope coupling in giant stars we can explain the initial spins of pulsars.

Export citation and abstract BibTeX RIS

Please wait… references are loading.
10.1086/306153