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Planetary nebulae in Local Group galaxies. IX. Velocity modulated photographs of the center of M31.

Abstract

A sequence of velocity-modulated photographs made with a camera consisting of a temperature-tuned, 2.1 A (FWHM) O III forbidden line 5007 A interference filter, a two-stage cooled image intensifier, and a calibrating photomultiplier, was used to find and measure the radial velocities of 42 faint planetary nebulae in the center of M31. Of the 42, 19 are new identifications. After deriving a planetary-to-luminosity ratio (PLR) value of 69 + or - 9 for the luminosity corresponding to an integrated blue magnitude of 8.37, the PLR is combined with M31's integrated magnitude to estimate that there are approximately 2800 + or - 350 nebulae in the first 3 mag of M31's luminosity function, and 21,000 planetary nebulae within 8 mag of the brightest nebulae.


Publication:
The Astrophysical Journal
Pub Date:
May 1982
DOI:

10.1086/159889

Bibcode:
1982ApJ...256..120L
Keywords:
  • Andromeda Galaxy;
  • Astronomical Photography;
  • Galactic Clusters;
  • Galactic Structure;
  • Local Group (Astronomy);
  • Planetary Nebulae;
  • Radial Velocity;
  • Velocity Modulation;
  • Brightness;
  • Interstellar Extinction;
  • Luminosity;
  • Magellanic Clouds;
  • Star Distribution;
  • Stellar Evolution;
  • Astronomy
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