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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

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

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