Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2024-12-27T05:05:46.876Z Has data issue: false hasContentIssue false

The radial velocity variations of WR46 (WN3p)

Published online by Cambridge University Press:  07 August 2017

V.S. Niemela
Affiliation:
1 Institute de Astronomía y Física del Espacio, Buenos Aires, Argentina
R.H. Barbá
Affiliation:
2 Observatorio Astronómico, Universidad National de La Plata, Argentina
M.M. Shara
Affiliation:
3 Space Telescope Science Institute, Baltimore, USA

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.

Spectral observations of the WN3p star WR46 (HD 104994) obtained during June 1993 and January/February 1994 display large amplitude radial velocity variations of the strong emission lines Nv 4603-19Å and HeII 4686A, on a time scale of a fraction of a day. The most probable period found is 0.311 d, similar to the photometric period found by previous authors. The amplitude of the radial velocity variations of Nv emission is almost twice that of HeII. Noting the similarity of WR46 with low mass X-ray binaries, we suggest that the emission line spectrum corresponds to that of a luminous accretion disk in an evolved binary system.

Type
Session IV - poster summaries
Copyright
Copyright © Kluwer 1995 

References

Cowley, A.P., Schmidtke, P.C., Hutchings, J.B., Crampton, D., McGrath, T.K. 1993, ApJ (Letters) 418, L63 CrossRefGoogle Scholar
van Genderen, A.M., van der Hucht, K.A., Larsen, I. 1990, A&A 229, 123 Google Scholar
van Genderen, A.M., Verheijen, M.A.W., van der Hucht, K.A. et al. 1991, in: van der Hucht, K.A. & Hidayat, B. (eds.), Wolf-Rayet Stars and Interrelations with Other Massive Stars in Galaxies, Proc. IAU Symp. No. 143 (Dordrecht: Kluwer), p. 129 Google Scholar
Mathewson, D.S., Ford, V.L. 1970, Mem. RAS 74, 139 Google Scholar
Pollock, A.M.T. 1987, ApJ 320, 283 Google Scholar