Hostname: page-component-669899f699-vbsjw Total loading time: 0 Render date: 2025-04-25T18:05:04.320Z Has data issue: false hasContentIssue false
  • English
  • Français

Changes in Emission Line Intensities of HBV475

Published online by Cambridge University Press:  22 September 2016

Shin'ichi Tamura
Shin'ichi Tamura*
Affiliation:
Astronomical Institute, Tohoku University, Sendai, JAPAN

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.

Some of the results in the spectroscopic observation of HBV475 are presented.

Type
Session VIII: Planetary Nebulae and Their Influence on the Galaxy
Information
Symposium - International Astronomical Union , Volume 76: Planetary Nebulae , 1978 , pp. 357
Copyright
Copyright © Reidel 1978