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| Query : 2004MNRAS.354L...1L |
2004MNRAS.354L...1L - Mon. Not. R. Astron. Soc., 354, L1-L6 (2004/October-2)
The nearest extreme starburst: bubbles, young star clusters and outflow in the merger NGC 3256.
LIPARI S.L., DIAZ R.J., FORTE J.C., TERLEVICH R., TANIGUCHI Y., AGUERO M.P., ALONSO-HERRERO A., MEDIAVILLA E. and ZEPF S.
Abstract (from CDS):
The first analysis of the spatial distribution of young star cluster candidates shows that more than 90 per cent of them are located in a complex starburst structure, including some of the bubble walls, three nuclei and three blue asymmetrical spiral arms.
We have made a kinematic study of the ionized gas in the core of the main optical nucleus, performed with HST STIS spectra. The shape of the rotation curve and the emission-line profile can be explained by the presence in the core of young star clusters with outflow. Any low-luminosity active galactic nucleus associated with this core would have a mass less than 107 M☉. It is also probable that the compact X-ray and radio emission of ULX(7)N - the source coincident with the main optical nucleus - is the result of a few recent supernova remnants.
Abstract Copyright: 2004 RAS
Journal keyword(s): supernovae: general - ISM: bubbles - galaxies: individual: NGC 3256 - galaxies: interactions - galaxies: kinematics and dynamics - galaxies: star clusters
Nomenclature: Fig.1: [LDF2004] Shell A (Nos A-D).
CDS comments: ULX (7) N = [LWZ2002] 7 (N), ULX (13) = [LWZ2002] 13, regions RN and Arms = [LDT2000] objects.
Simbad objects: 19
| Number of rows : 19 |
| 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 2623 | LIN | 08 38 24.016 | +25 45 16.29 | 14.10 | 13.99 | 13.36 | ~ | 533 | 2 | ||
| 2 | M 82 | AGN | 09 55 52.430 | +69 40 46.93 | 9.61 | 9.30 | 8.41 | ~ | 6156 | 6 | ||
| 3 | [EF2003] B6 | HII | 10 27 50.1 | -43 54 22 | ~ | 3 | 0 | |||||
| 4 | [LDT2000] R09 | X | 10 27 51.23 | -43 54 10.9 | ~ | 5 | 0 | |||||
| 5 | NGC 3256 | Sy2 | 10 27 51.284 | -43 54 13.55 | 11.83 | 11.33 | 10.62 | 11.9 | ~ | 920 | 2 | |
| 6 | [LDT2000] R08 | X | 10 27 51.64 | -43 54 09.7 | ~ | 5 | 0 | |||||
| 7 | [LDT2000] R02 | X | 10 27 51.76 | -43 54 13.6 | ~ | 5 | 0 | |||||
| 8 | [LDT2000] R04 | X | 10 27 52.03 | -43 54 12.6 | ~ | 5 | 0 | |||||
| 9 | [EF2003] B3 | HII | 10 27 52.88 | -43 54 11.8 | ~ | 5 | 0 | |||||
| 10 | NGC 4038 | EmG | 12 01 53.002 | -18 52 03.32 | 10.91 | 9.74 | 11.0 | ~ | 1364 | 1 | ||
| 11 | NAME Antennae | IG | 12 01 53.170 | -18 52 37.92 | ~ | 1749 | 0 | |||||
| 12 | NGC 4039 | GiP | 12 01 53.51 | -18 53 10.3 | 11.08 | 9.77 | ~ | 1173 | 1 | |||
| 13 | [LDT2000] R01 | HII | ~ | ~ | ~ | 3 | 0 | |||||
| 14 | [LDT2000] Arm III | PoG | ~ | ~ | ~ | 3 | 0 | |||||
| 15 | [LDT2000] R03 | PoG | ~ | ~ | ~ | 2 | 0 | |||||
| 16 | [LDT2000] Arm I | PoG | ~ | ~ | ~ | 3 | 0 | |||||
| 17 | [LDT2000] R06 | PoG | ~ | ~ | ~ | 3 | 0 | |||||
| 18 | [LDT2000] R10 | PoG | ~ | ~ | ~ | 3 | 0 | |||||
| 19 | [LDT2000] Arm II | PoG | ~ | ~ | ~ | 3 | 0 |
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