Hostname: page-component-848d4c4894-mwx4w Total loading time: 0 Render date: 2024-06-25T02:28:11.498Z Has data issue: false hasContentIssue false
  • English
  • Français

The dynamics of PNe halos and the timescale correlation distance

Published online by Cambridge University Press:  25 May 2016

Arsen R. Hajian ,
Adam Frank ,
Bruce Balick  and
Yervant Terzian
Arsen R. Hajian
Affiliation:
1United States Naval Observatory
Adam Frank
Affiliation:
2University of Minnesota
Bruce Balick
Affiliation:
3University of Washington
Yervant Terzian
Affiliation:
4Cornell University

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.

We present deep narrow-band CCD images of four PNe obtained with the Palomar 5-m telescope in the light of [N II]λ6584 + Hα and [O III]λ5007. Several previously undetected structures are found, including faint multiple envelope structures. The inclusion of these sources with data for other multiple envelope PNe published in the literature permit an evaluation of the relationship between PNe ‘shells’ and the thermal pulses of the PN nucleus.

Type
II. Distances to Galactic Planetary Nebulae
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 47
Copyright
Copyright © Kluwer 1997 

References

Frank, A., van der Veen, W. E. C. J. & Balick, B. 1994, A&A, 282, 554.Google Scholar
Hajian, A.R., Frank, A., Balick, B. & Terzian, Y. 1997, ApJ, in press.Google Scholar
Stanghellini, L. & Pasquali, A. 1995, ApJ, 452, 286.CrossRefGoogle Scholar
Vassiliadis, E. & Wood, P. R. 1994, ApJS, 92, 125.Google Scholar