VDB 113
(vdBergh 113; MWSC 2819)
0.87
UTI
0.75
CN
1.0
Cdens
1.0
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
6.2 [arcmin]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
VDB 113 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very massive, near-solar metallicity, young cluster (see Parameters). It is well-studied in the literature.
Note: This object shares a significant percentage of members with 2 later reported entries. See table with shared members information.
Relatively close
Moderate extinction
Very massive
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 272.174 | -21.45 | 0.662 | -0.73 | -1.397 | -35.75 |
| Hunt & Reffert | 2024 | 272.165 | -21.441 | 0.654 | -0.719 | -1.423 | -38.175 |
| Cavallo et al. | 2024 | 272.234 | -21.453 | 0.657 | â | â | â |
| Hunt & Reffert | 2023 | 272.165 | -21.441 | 0.654 | -0.719 | -1.423 | -38.175 |
| Just et al. | 2023 | 272.167 | -21.406 | â | â | â | â |
| Kharchenko et al. | 2016 | 272.167 | -21.406 | â | â | â | â |
| Dias et al. | 2014 | 272.15 | -21.417 | â | -1.76 | -1.98 | â |
| Kharchenko et al. | 2013 | 272.175 | -21.405 | â | -0.35 | -3.15 | -8.0 |
| Gozha et al. | 2012 | 272.15 | -21.417 | â | â | â | â |
| Piskunov et al. | 2008 | 272.209 | -21.424 | â | â | â | â |
| Kharchenko et al. | 2007 | 272.14 | -21.42 | â | 0.23 | â | -16.0 |
| Piskunov et al. | 2007 | 272.209 | -21.424 | â | â | â | â |
| Kharchenko et al. | 2005 | 272.22 | -21.42 | â | -0.26 | -2.47 | -16.0 |
| Kharchenko et al. | 2003 | 272.17 | -21.44 | â | -0.42 | -2.3 | â |
| Dias et al. | 2002 | 272.15 | -21.417 | â | -1.76 | -1.98 | -16.0 |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 742* | â | â |
| Cavallo et al. | 2024 | 1.19 | 2.53 | â | 50 | -0.160 | â | â | â |
| Hunt & Reffert | 2023 | 1.41 | 1.96 | 2.65 | 35 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 200 | â | 484 | â | â |
| Kharchenko et al. | 2016 | 2.06 | 3.23 | â | 200 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.06 | 3.23 | â | 200 | -0.358 | â | â | â |
| Gozha et al. | 2012 | 1.67 | â | â | 32 | â | 69183 | â | â |
| Piskunov et al. | 2008 | 3.47 | 1.80 | â | 32 | â | 45186* | â | â |
| Piskunov et al. | 2007 | 3.47 | 1.80 | â | 32 | â | 6471 | â | â |
| Kharchenko et al. | 2005 | 3.47 | 1.80 | â | 32 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.67 | 0.78 | â | â | â | â | â | â |
| Dias et al. | 2002 | 3.47 | 1.80 | â | 32 | -0.358 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.