Hostname: page-component-76fb5796d-2lccl Total loading time: 0 Render date: 2024-04-27T08:36:20.308Z Has data issue: false hasContentIssue false
  • English
  • Français

IRAS 21282+5050: A Transitional Planetary Nebula

Published online by Cambridge University Press:  12 April 2016

L. Likkel ,
M. Morris ,
A. Omont  and
T. Forveille
L. Likkel
Affiliation:
UCLA
M. Morris
Affiliation:
UCLA
A. Omont
Affiliation:
Grenoble
T. Forveille
Affiliation:
Grenoble

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.

IRAS 21282+5050 is very compact planetary nebula with a substantial molecular shell. It is carbon-rich and exhibits infrared features attributed to PAH molecules. It has a far infrared color temperature higher than almost all other planetary nebulae, with IRAS flux ratios similar to low color temperature evolved stars. We present VLA images of IRAS 21282 at wavelengths of 2 and 6 cm (with FWHM beamsizes of 0.5” and 0.9”, respectively).

Type
3. Evolution of Peculiar Red Giant Stars
Information
International Astronomical Union Colloquium , Volume 106: Evolution of Peculiar Red Giant Stars , 1989 , pp. 233
Copyright
Copyright © Cambridge University Press 1989

References

1 Cohen, M. and Jones, B. 1987, Ap. J. Lett. 321, L151.Google Scholar
2 Likkel, L., Forveille, T., Omont, A., and Morris, M. 1988, Astron. Ap., in press.Google Scholar
3 de Muizon, m., Geballe, T.R., D'Hendecourt, L.B., and VBaas, F. 1986, Astrophvs. J. Letters 306, L105.Google Scholar