Hostname: page-component-848d4c4894-v5vhk Total loading time: 0 Render date: 2024-07-07T13:26:59.907Z Has data issue: false hasContentIssue false
  • English
  • Français

Study of photometric and spectral variability of Planetary Nebulae during 1968–1996

Published online by Cambridge University Press:  25 May 2016

E. B. Kostyakova
E. B. Kostyakova*
Affiliation:
Sternberg Astronomical Institute, Moscow, Russia

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 photometric and spectral study of 7 selected planetary nebulae has been carried out since 1968. (See: Mem. Soc. Roy. Sci. Liege, 6e ser., 1973, 5, 473). During nearly 30 years of photoelectric observations, 5 planetaries (NGC 6572, IC 4997, Hu2-1, NGC 6891 and NGC 6543) have undergone noticeable variations of integral UVB-brightness in the range 0.1÷0.6 mag. The nebulae NGC 6720 and IC 3568 showed no changes of integral brightness exceeding 0.1 mag. The most remarkable behaviour was found for the nebula IC 4997: a steady decrease of the integral brightness in 1968–85, amounted on the whole to 0.4 ÷ 0.6 mag., an unexpected stop of this decrease in 1985–86, and almost monotonous brightening in 1987–96.

Type
IV. Envelopes
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 251
Copyright
Copyright © Kluwer 1997 

References

Publ. of Sternberg Astron. Inst., 1991, 62, 143.Google Scholar
Sov. Astron. J. Lett., 1990, 16, 12, 1085.Google Scholar
Sov. Astron. J. Lett., 1994, 20, 2, 122.Google Scholar