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| Query : 1992BAAS...24.1192B |
1992BAAS...24.1192B - Bull. American Astron. Soc., 24, 1192 (1992)
Why do head tail sources exist in poor clusters of galaxies ?
BATUSKI D.J., VENKATESAN T.C.A., HANISCH R.J. and BURNS J.O.
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 | NGC 742 | GiP | 01 56 24.1660196952 | +05 37 36.049925676 | 14.8 | ~ | 57 | 0 | ||||
| 2 | NGC 1044 | rG | 02 41 06.183 | +08 44 16.72 | 14.8 | ~ | 72 | 1 | ||||
| 3 | NGC 1265 | rG | 03 18 15.674 | +41 51 27.94 | 14.7 | ~ | 386 | 2 | ||||
| 4 | NGC 4055 | rG | 12 04 01.4688806232 | +20 13 56.324233308 | 14.4 | ~ | 125 | 1 | ||||
| 5 | NGC 7503 | rG | 23 10 42.2807650944 | +07 34 03.752239404 | 14.9 | ~ | 76 | 1 |
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