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Consequences of a New Distance Determination of 3C58

Published online by Cambridge University Press:  04 August 2017

D. A. Green  and
S. F. Gull
D. A. Green
Affiliation:
Mullard Radio Astronomy Observatory, Cavendish Laboratory, Cambridge, United Kingdom
S. F. Gull
Affiliation:
Mullard Radio Astronomy Observatory, Cavendish Laboratory, Cambridge, United Kingdom

Extract

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In this paper we present new observations that show 3C58 is much closer than has been assumed in the past. This necessitates a reappraisal of many of the quantitative comparisons that have been made between 3C58 and the Crab Nebula or other ‘filled-centre’ remnants.

Type
III. Center Filled Morphologies
Information
Symposium - International Astronomical Union , Volume 101: Supernova Remnants and Their X-Ray Emission , 1983 , pp. 335 - 340
Copyright
Copyright © Reidel 1983 

References

Albinson, J.S. & Gull, S.F., 1982. ‘Regions of Recent Star Formation’, (eds. Roger, R.S. & Dewdney, P.E.), p. 193, (Reidel).Google Scholar
Becker, R.H., Helfand, D.J. & Szymkowiak, A.E., 1982. Astrophys. J., 255, 557.Google Scholar
Roberts, W.W., 1972. Astrophys. J., 173, 259.Google Scholar
Schmidt, M., 1955. In ‘Stars and Stellar Systems Vol. 5’, (eds. Blaaw, A. & Schmidt, M.), p. 513, (Univ. of Chicago Press).Google Scholar
Spitzer, L., 1978. ‘Physical Processes in the Interstellar Medium’, (Wiley).Google Scholar
Stephenson, F.R., 1971. Quart. J. R. astr. Soc., 12, 10.Google Scholar
Weaver, H. & Williams, D.R.W., 1973. Astr. Astrophys. Suppl. Ser., 8, 1.Google Scholar
Williams, D.R.W., 1973a. Astr. Astrophys. Suppl. Ser., 8, 505.Google Scholar
Williams, D.R.W., 1973b. Astr. Astrophys. 28, 309.Google Scholar