Archival HST study of novae. I. The Seyfert galaxy NGC 3627

Abstract

A V-band nova search was carried out in NGC 3627 with archival Hubble Space Telescope WFPC2 data which was obtained in the period between November 1997 and January 1998. A total of four novae candidates were discovered which corresponds to a global nova rate of R = 83.65 ± 7.58 yr ^-1. Taking into account the K-band luminosity obtained from 2MASS ( Jarrett et al., 2003) yielded a luminosity specific nova rate (LSNR) of ν_K = 9.60 ± 1.64 novae per year per 10 ¹⁰L_{⊙, K}. Excluding one of the candidates which may be a long-period variable leads to a LSNR of ν_K = 7.20 ± 1.23 novae per year per 10 ¹⁰L_{⊙, K}. These values are higher than other known nova rates for external galaxies except the Magellanic Clouds.