A HUBBLE SPACE TELESCOPE SURVEY FOR NOVAE IN M87. I. LIGHT AND COLOR CURVES, SPATIAL DISTRIBUTIONS, AND THE NOVA RATE
Authors: Michael M. Shara, Trisha F. Doyle, Tod R. Lauer, David Zurek, J. D. Neill, Juan P. Madrid, Joanna Mikołajewska, D. L. Welch, and Edward A. Baltz
2016 The Astrophysical Journal Supplement Series2271.
Provider: AAS Journals
Caption: Figure 1.
A map of the locations of 32 classical novae (numbers 1–32) in M87 overlaid on the full drizzled HST ACS/WFC V band image. Nine fainter variables (numbered 33–41), which are too blue to be Miras, are likely to be very slow and/or symbiotic novae.