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| Query : 1992MmSAI..63..233R |
1992MmSAI..63..233R - Mem. Soc. Astron. Ital., 63, 233-241 (1992)
The use of nebular spectra of type IA. Supernovae for distance determinations. The distance to the Centaurus group.
RUIZ-LAPUENTE P., LUCY L.B. and DANZIGER I.J.
Journal keyword(s):
Simbad objects: 5
| Number of rows : 5 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | ACO 3526 | ClG | 12 48 49.2 | -41 18 17 | ~ | 1154 | 2 | |||||
| 2 | NAME Centaurus A | BLL | 13 25 27.61521044 | -43 01 08.8050291 | 8.18 | 6.84 | 6.66 | ~ | 4774 | 3 | ||
| 3 | SN 1986G | SN* | 13 25 36.46 | -43 01 53.6 | 12.45 | 11.44 | SNIapec | 422 | 1 | |||
| 4 | SN 1972E | SN* | 13 39 52.7 | -31 40 09 | 8.49 | 8.30 | SNIa | 309 | 1 | |||
| 5 | NGC 5253 | rG | 13 39 55.990 | -31 38 24.11 | 11.48 | 10.94 | 10.49 | 10.33 | 13.47 | ~ | 1421 | 4 |
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