Hostname: page-component-54dcc4c588-gwv8j Total loading time: 0 Render date: 2025-10-14T08:17:56.400Z Has data issue: false hasContentIssue false
  • English
  • Français

A Search for Optical-UV Fading of Central Stars

Published online by Cambridge University Press:  07 August 2017

B. Altner  and
S.R. Heap
B. Altner
Affiliation:
Applied Research Corporation (ARC), Landover, MD USA
S.R. Heap
Affiliation:
Laboratory for Astronomy and Solar Physics NASA Goddard Space Flight Center, Greenbelt, MD USA

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.

We derive estimates of the masses of planetary nebulae central stars (CSPN), based on their rate of optical-UV fading.

Information

Type
V. Planetary Nebulae Connection: Evolution to White Dwarfs
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 485
Copyright
Copyright © Kluwer 1993