VDBH 139
(Hogg 15; MWSC 2063; OCL 891; vdBergh-Hagen 139; ESO 095 15)
0.91
UTI
0.79
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
3.2 [arcmin]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
VDBH 139 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, very young cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is very well-studied in the literature.
Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.
Distant
High extinction
Massive
Metal-rich
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 190.902 | -63.101 | 0.281 | -6.033 | -0.463 | -8.203 |
| Hunt & Reffert | 2024 | 190.912 | -63.102 | 0.287 | -6.038 | -0.453 | -26.45 |
| Celli et al. | 2024 | 190.906 | -63.101 | β | β | β | β |
| Cavallo et al. | 2024 | 190.907 | -63.103 | 0.288 | β | β | β |
| Hunt & Reffert | 2023 | 190.912 | -63.102 | 0.287 | -6.038 | -0.453 | -26.45 |
| Just et al. | 2023 | 190.888 | -63.095 | β | β | β | β |
| Jaehnig et al. | 2021 | 190.89 | -63.1 | 0.289 | -6.031 | -0.471 | β |
| Rain et al. | 2021 | 190.906 | -63.101 | 0.266 | -6.018 | -0.461 | β |
| Cantat-Gaudin et al. | 2020 | 190.906 | -63.101 | 0.266 | -6.018 | -0.461 | β |
| SΓ‘nchez et al. | 2020 | 190.904 | -63.1 | β | -5.854 | -0.404 | β |
| Cantat-Gaudin & Anders | 2020 | 190.906 | -63.101 | 0.266 | -6.018 | -0.461 | β |
| Soubiran et al. | 2018 | 190.906 | -63.101 | β | β | β | -23.09 |
| Bica et al. | 2019 | 190.888 | -63.098 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 190.906 | -63.101 | 0.266 | -6.018 | -0.461 | β |
| Loktin & Popova | 2017 | 190.905 | -63.1 | β | -15.131 | -2.329 | 55.0 |
| Kharchenko et al. | 2016 | 190.888 | -63.095 | β | β | β | β |
| Dias et al. | 2014 | 190.904 | -63.1 | β | -3.86 | -2.51 | β |
| Kharchenko et al. | 2013 | 190.897 | -63.098 | β | -6.55 | -1.0 | 55.0 |
| van den Bergh | 2006 | 190.9 | -63.1 | β | β | β | β |
| Dias et al. | 2002 | 190.904 | -63.1 | β | -7.87 | 2.39 | 55.0 |
π‘ 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 | β | β | β | β | β | 2408* | β | β |
| Celli et al. | 2024 | β | β | β | 2 | β | 1064 | β | β |
| Cavallo et al. | 2024 | 3.18 | 3.66 | β | 20 | 0.730 | β | β | β |
| Hunt & Reffert | 2023 | 3.24 | 4.07 | 2.75 | 9 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 4 | β | 311 | β | β |
| Jaehnig et al. | 2021 | 3.38* | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 3.39 | 4.03 | β | 4 | β | β | β | 0 |
| Cantat-Gaudin et al. | 2020 | 3.02 | 3.40 | β | 2 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 3.39 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 3.39 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 3.39 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 2.42 | 3.47 | β | 7 | β | β | β | β |
| Kharchenko et al. | 2016 | 3.08 | 3.94 | β | 4 | β | β | β | β |
| Kharchenko et al. | 2013 | 3.08 | 3.94 | β | 4 | β | β | β | β |
| van den Bergh | 2006 | 2.26 | 3.38 | β | 6 | β | β | β | β |
| Dias et al. | 2002 | 3.20 | 4.03 | β | 4 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Silver sample.