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Variable “cool” central stars of planetary nebulae

  • G. Handler
Published/Copyright: March 16, 2017
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Open Astronomy
From the journal Open Astronomy Volume 4 Issue 3

Published Online: 2017-3-16
Published in Print: 1995-9-1

© 2017

Articles in the same Issue

  1. Contents
  2. XCOV12: a report on the L19-2 campaign
  3. G29-38 and asteroseismology of cool DA white dwarfs
  4. HST observations of the DAV white dwarf G 226-29
  5. The DBV stars: progress and problems
  6. GD 358 in 1994: a progress report
  7. The PNN and PG 1159 connection
  8. Timescale for the variation of the 539 s pulsation mode of PG 1159-035
  9. Spectra of GW Vir type pulsators
  10. Theoretical and observed periods of the pulsating pre-white dwarfs
  11. NGC 2452: luminosity variations of the PN nucleus?
  12. Variable “cool” central stars of planetary nebulae
  13. RXJ 2117+34: preliminary results of the August 1994 WET campaign
  14. The AM CVn type stars: an overview
  15. Observations of modulation amplitude colors in AM CVn
  16. The secondary star in AM CVn
  17. Period stability in AM CVn
  18. A 3-D SPH model of helium accreation disks in the interacting binary white dwarf systems AM CVn and EC 15330-1403
  19. The AM CVn trial: the case for superhumps
https://doi.org/10.1515/astro-1995-0312
Creative Commons
BY-NC-ND 4.0

Articles in the same Issue

  1. Contents
  2. XCOV12: a report on the L19-2 campaign
  3. G29-38 and asteroseismology of cool DA white dwarfs
  4. HST observations of the DAV white dwarf G 226-29
  5. The DBV stars: progress and problems
  6. GD 358 in 1994: a progress report
  7. The PNN and PG 1159 connection
  8. Timescale for the variation of the 539 s pulsation mode of PG 1159-035
  9. Spectra of GW Vir type pulsators
  10. Theoretical and observed periods of the pulsating pre-white dwarfs
  11. NGC 2452: luminosity variations of the PN nucleus?
  12. Variable “cool” central stars of planetary nebulae
  13. RXJ 2117+34: preliminary results of the August 1994 WET campaign
  14. The AM CVn type stars: an overview
  15. Observations of modulation amplitude colors in AM CVn
  16. The secondary star in AM CVn
  17. Period stability in AM CVn
  18. A 3-D SPH model of helium accreation disks in the interacting binary white dwarf systems AM CVn and EC 15330-1403
  19. The AM CVn trial: the case for superhumps
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