| (Neill+Shara, 2005) | Details on Acronym: [NS2005] | |
| [NS2005] | ||
| Write: | <<[NS2005] NGC 205 N>> <<[NS2005] M 32 Star A>> <<[NS2005] NGC 205 Star A>> | |
| N: | 1+1+3 | |
| Object: | * (SIMBAD class: Star) | |
| Stat: | is completely incorporated in Simbad | |
| Note: | Optical imaging at the 0.8m Tenagra telescope. Use of HST archival data. Discovery of a new nova candidate in NGC 205. Nova 1 in M 32 is already defined, see [NT2004]. Figs 7, 8: Stars in the field of the 2 novae. | |
| in source: | NGC 205 = M 110 | |
| in source: | M 32 = NGC 221 | |
| Ref: | =2005AJ....129.1873N | |
| by | NEILL J.D. , SHARA M.M. | |
| Astron. J., 129, 1873-1885 (2005) | ||
| A possible high nova rate for two Local Group dwarf galaxies: M32 and NGC 205. | ||
| o | M 32 Nova 1 = [NT2004] J004244.991+405304.76 | |
| o | Table 2: <[NS2005] NGC 205 N> (No. 1). Fig.7: <[NS2005] M 32 Star A> (No. A). Fig8: <[NS2005] NGC 205 Star A> (Nos A-C). | |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database | |