Observations of NOVAE in M51, M87, and M101: A Preliminary Report

  • A. W. Shafter
  • R. Ciardullo
  • C. J. Pritchet
Part of the Astrophysics and Space Science Library book series (ASSL, volume 208)

Abstract

We report preliminary results from a new program of observations of novae in nearby galaxies. The principal goal of the program is to explore the population of nova progenitors through observations of galaxies having a wide range of Hubble types. Here we present preliminary results from observations of the spiral systems M51 and M101, and the giant elliptical, M87. Based on available data, we find no evidence that the luminosity specific nova rate varies across the Hubble sequence.

Keywords

Stellar Population Planetary Nebula Nearby Galaxy Single Epoch Hubble Type 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Kluwer Academic Publishers 1996

Authors and Affiliations

  • A. W. Shafter
    • 1
  • R. Ciardullo
    • 2
  • C. J. Pritchet
    • 3
  1. 1.Dept. of AstronomySan Diego State UnivSan DiegoUSA
  2. 2.Dept. of Astronomy & AstrophysicsPenn State UnivUniversity ParkUSA
  3. 3.Dept. of PhysicsUniv. of VictoriaVictoriaCanada

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