Hostname: page-component-848d4c4894-x5gtn Total loading time: 0 Render date: 2024-06-01T05:24:29.583Z Has data issue: false hasContentIssue false
  • English
  • Français

Radial Velocity of the Central Star of NGC 1514

Published online by Cambridge University Press:  14 August 2015

A. Mammano ,
R. Margoni  and
M. Perinotto
A. Mammano
Affiliation:
Asiago Astrophysical Observatory, Italy
R. Margoni
Affiliation:
Asiago Astrophysical Observatory, Italy
M. Perinotto
Affiliation:
Asiago Astrophysical Observatory, 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.

We would like to report on some spectroscopic observations made of the central star of the planetary nebula NGC 1514, which we think can support the binary hypothesis now advanced by Kohoutek.

Type
Session V – Central Stars
Information
Symposium - International Astronomical Union , Volume 34: Planetary Nebulae , 1968 , pp. 329
Copyright
Copyright © Reidel 1968