Hostname: page-component-6bf8c574d5-7jkgd Total loading time: 0 Render date: 2025-02-22T10:49:04.827Z Has data issue: false hasContentIssue false
  • English
  • Français

Quantitative Investigations on Mass Outflow from Planetary Nebulae Nuclei

Published online by Cambridge University Press:  19 July 2016

S. Cerrato ,
L. Bianchi ,
M. Grewing ,
M. Bässgen  and
G. Bässgen
S. Cerrato
Affiliation:
Astronomisches Institut, Universität Tübingen (FRG)
L. Bianchi
Affiliation:
Osservatorio Astronomico di Torino (Italy)
M. Grewing
Affiliation:
Astronomisches Institut, Universität Tübingen (FRG)
M. Bässgen
Affiliation:
Astronomisches Institut, Universität Tübingen (FRG)
G. Bässgen
Affiliation:
Astronomisches Institut, Universität Tübingen (FRG)

Abstract

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.

Observed P-Cygni line profiles in the UV spectra of central stars of Planetary Nebulae (PNN) obtained with the IUE satellite has been fitted by theoretical profiles in order to determine mass loss rates.

Type
III. Central Stars
Information
Symposium - International Astronomical Union , Volume 131: Planetary Nebulae , 1989 , pp. 318
Copyright
Copyright © Kluwer 1989