VDB 130
(vdBergh 130)
Summary
VDB 130 is a rich, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It is well-studied in the literature.
This object shares a very small percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 304.425 | 39.35 | – | -3.61 | -4.58 | – |
| Kharchenko et al. (2012) | 304.425 | 39.35 | – | -2.22 | -4.39 | – |
| Loktin & Popova (2017) | 304.425 | 39.35 | – | -1.002 | -1.194 | – |
| Dias et al. (2021) | 304.462 | 39.34 | 0.521 | -3.609 | -5.075 | – |
| Hunt & Reffert (2023) | 304.517 | 39.367 | 0.581 | -3.548 | -5.127 | -8.7 |
| He et al. (2023) | 304.555 | 39.385 | 0.579 | -3.62 | -5.078 | -18.44 |
| Cavallo et al. (2024) | 304.588 | 39.368 | 0.578 | – | – | – |
| Hunt & Reffert (2024) | 304.517 | 39.367 | 0.581 | -3.548 | -5.127 | -8.7 |
| Almeida et al. (2025) | 304.462 | 39.34 | – | – | – | – |
| UCC | 304.512 | 39.356 | 0.571 | -3.587 | -5.154 | -23.664 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.916, Dist=1589.0, Age=7.4 |
| Kharchenko et al. (2012) | e_bv=0.916, distance=1589, log_age=7.4 |
| Loktin & Popova (2017) | E(B-V)=0.63, Dist=2179, logt=8.08 |
| Dias et al. (2021) | Av=2.356, Dist=1456, logage=6.974, [Fe/H]=-0.029 |
| Hunt & Reffert (2023) | AV50=2.433, diffAV50=2.574, MOD50=11.144, logAge50=6.661 |
| He et al. (2023) | A0=2.95, m-M=11.35, logA=6.5 |
| Cavallo et al. (2024) | AV50=1.67, dMod50=11.04, logAge50=7.42, [Fe/H]50=0.31 |
| Hunt & Reffert (2024) | MassJ=906.565, MassTot=906.565 |
| Almeida et al. (2025) | AV=2.356, Dist=1456, logAge=6.974, MassRk=380.1 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Teutsch 305 | 0.7 | 304.33 | 39.63 | 0.36 | -3.57 | -5.43 | – | 0.12 |