Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-06T06:19:52.762Z Has data issue: false hasContentIssue false
  • English
  • Français

Physical Conditions and Abundances in Abell 30

Published online by Cambridge University Press:  26 May 2016

R. Wesson ,
X-W. Liu  and
M. J. Barlow
R. Wesson
Affiliation:
Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT
X-W. Liu
Affiliation:
Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT
M. J. Barlow
Affiliation:
Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT

Extract

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.

Abell 30 is one of a small number of PN known as born-again PN, which appear to be old nebulae whose central star has undergone a further ejection of highly processed material. It consists of a large, faint, spherical shell, in which several bright knots are embedded. The knots were first noted by Jacoby (1979), and analysis of their abundances by Hazard et al (1980) and Jacoby & Ford (1983) showed that they are extremely hydrogen-deficient.

Type
Part VI: The Ionized Gas in Planetary Nebulae
Information
Symposium - International Astronomical Union , Volume 209: Planetary Nebulae: Their Evolution and Role in the Universe , 2003 , pp. 381 - 382
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Greenstein, J.L. 1981, ApJ, 245, 124 CrossRefGoogle Scholar
Hazard, C., Terlevich, R., Ferland, G. et al. 1980 Nature, 285, 463 Google Scholar
Jacoby, G.H. 1979, ApJS, 42, 1 CrossRefGoogle Scholar
Jacoby, G.H., & Ford, H.C. 1983, ApJ, 266, 298 Google Scholar
Jacoby, G.H., & Chu, Y-H. 1989, IAUS, 131, 183 Google Scholar
Kingsburgh, R.L., & Barlow, M.J. 1994, MNRAS, 271, 257 Google Scholar
Liu, X-W., Storey, P.J., Barlow, M.J. et al. 2000, MNRAS, 312, 585 Google Scholar
Liu, X-W., Luo, S-G., Barlow, M.J. et al. 2001, MNRAS, 327, 141 CrossRefGoogle Scholar