Hostname: page-component-cb9f654ff-pvkqz Total loading time: 0 Render date: 2025-08-27T19:18:50.112Z Has data issue: false hasContentIssue false
  • English
  • Français

P Cygni profiles variability in central stars of Planetary Nebulae

Published online by Cambridge University Press:  25 May 2016

P. Patriarchi  and
M. Perinotto
P. Patriarchi
Affiliation:
1Gruppo Nazionale di Astronomia del CNR, UdR di Arcetri
M. Perinotto
Affiliation:
2Dipartimento di Astronomia e Scienza dello Spazio, Univ. di Firenze

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 variability of P Cygni profiles is important because of its connection with the mechanism of wind production and with the behaviour of the associated mass loss rates.

Information

Type
III. Central Stars
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 125
Copyright
Copyright © Kluwer 1997