Hostname: page-component-cd9895bd7-7cvxr Total loading time: 0 Render date: 2024-12-29T07:03:15.947Z Has data issue: false hasContentIssue false
  • English
  • Français

Mass Loss in Two Low Temperature Central Stars of Planetary Nebulae

Published online by Cambridge University Press:  07 August 2017

A. Modigliani ,
M. Perinotto  and
P. Patriarchi
A. Modigliani
Affiliation:
Dipartimento di Astronomia Univ. Firenze, L.go E. Fermi 5, I-50125 Firenze, Italy
M. Perinotto
Affiliation:
Dipartimento di Astronomia Univ. Firenze, L.go E. Fermi 5, I-50125 Firenze, Italy
P. Patriarchi
Affiliation:
GNA/CNR c/o Osserv. Arcetri, L.go E. Fermi 5, I-50125 Firenze, Italy

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.

The high resolution IUE images SWP 16742 and SWP 42675 have been studied to derive the fast wind properties of the central stars of the two low temperature planetary nebulae IC 2149 and Tc 1. The first image is from the IUE archive, while the second one has been taken by us.

Type
II. Highlights on the Nuclei
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 93
Copyright
Copyright © Kluwer 1993