Abstract
Optical velocity field mapping of G292.0+1.8 in the [0III] λ5007 Å line has been carried out using the IPCS with the 3.6 m ESO telescop_e at La Silla. Our data are not consistent with the suggestion that the [0III] emitting material in the western portion of this remnant is concentrated in an expanding ring. The existing data on G292.0+1.8 suggests that only the brightest portion of a thick shell of ejecta with high velocity spurs is observed. The expansion centroid, size, velocity and age of this SNR are derived.
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Clark, D.H., Tuohy, I.R., and Becker, R.H.: 1980, M.N.R.A.S. 193, 129
Goss, W.M., Shaver, P.A., Zealey, W.J., Murdin, P., and Clark, D.H.: 1979, M.N.R.A.S. 188, 357
Gull, S.F.: 1975, M.N.R.A.S. 171, 237
Lockhart, I.A., Goss, W.M., Caswell, J.L., and McAdam, W.B.: 1977, M.N.R.A.S. 179, 147
Murdin, P., and Clark, D.H.: 1979, M.N.R.A.S. 189, 501
Tuohy, I.R., Clark, D.H., and Burton, W.M.: 1982, Ap. J. 260, L56
White, R.L., and Long, K.S.: 1982, preprint
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1983 IAU
About this chapter
Cite this chapter
Braun, R., Goss, W.M., Danziger, I.J., Boksenberg, A. (1983). The Kinematics of the SNR G292.0+1.8. In: Danziger, J., Gorenstein, P. (eds) Supernova Remnants and their X-Ray Emission. International Astronomical Union / Union Astronomique Internationale, vol 101. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7231-5_22
Download citation
DOI: https://doi.org/10.1007/978-94-009-7231-5_22
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-277-1667-5
Online ISBN: 978-94-009-7231-5
eBook Packages: Springer Book Archive