Hostname: page-component-77c89778f8-m42fx Total loading time: 0 Render date: 2024-07-18T09:31:29.050Z Has data issue: false hasContentIssue false

The Masses of the Neutron Stars in M15C

Published online by Cambridge University Press:  25 May 2016

W.T.S. Deich
Affiliation:
Netherlands Foundation for Research in Astronomy, Postbus 2, 7990 AA Dwingeloo, The Netherlands
S.R. Kulkarni
Affiliation:
California Institute of Technology

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Several years of timing the pulsar in the binary neutron star system M15C have yielded the masses of both stars: the total mass is MT = 2.7121(6) M; the companion mass is mc = 1.36(4) M; and the pulsar mass is mp = 1.35(4) M. We argue that this system is not likely to have formed through accretion-induced collapse (AIC), and that the standard model also has problems in explaining the formation.

Type
4 Radio Pulsars
Copyright
Copyright © Kluwer 1996 

References

Anderson, S.B. et al. 1990, Nat 346, 42.CrossRefGoogle Scholar
Anderson, S.B., 1993, Ph.D. Thesis, California Institute of Technology.Google Scholar
Bailyn, C.D. & Grindlay, J.E. 1990, ApJ 353, 159.CrossRefGoogle Scholar
Bhattacharya, D. & Van den Heuvel, E.P.J. 1991, Phys. Rept. 203, 1.CrossRefGoogle Scholar
Burrows, A. & Woosley, S.E. 1986, ApJ 308, 680.Google Scholar
Flannery, B.P. & Van den Heuvel, E.P.J. 1975, A&A 39, 61.Google Scholar
Grindlay, J.E. & Bailyn, C.D. 1988, Nat 336, 48.Google Scholar
Nomoto, K. 1987 in The Origin and Evolution of Neutron Stars , IAU Symp. 125, Helfand, D.J. & Huang, J.H. (Eds.), Reidel, p. 281.CrossRefGoogle Scholar
Nomoto, K. & Kondo, Y. 1991, ApJ 367, L19.Google Scholar
Phinney, E.S. 1992, Phil. Trans. Roy. Soc. Lond. A341, 39.Google Scholar
Phinney, E.S. & Sigurdsson, S. 1991, Nat 349, 220.Google Scholar
Prince, T.A. et al. 1991, ApJ 374, L41.Google Scholar
Wolszczan, A. et al. 1989, Nat 337, 531.Google Scholar