Planetary nebulae in local group galaxies. IX - Velocity modulated photographs of the center of M31

Astronomy and Astrophysics – Astronomy

Scientific paper

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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

Scientific paper

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.

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