VDB 92
(FSR 1188; vdBergh 92; CMa06)
Summary
VDB 92 is a very rich, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is very 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) | 105.975 | -11.533 | – | -2.1 | 3.87 | 17.5 |
| Froebrich et al. (2007) | 106.0 | -11.579 | – | – | – | – |
| Piskunov et al. (2007) | 105.973 | -11.489 | – | – | – | – |
| Piskunov et al. (2008) | 105.973 | -11.489 | – | – | – | – |
| Loktin & Popova (2017) | 105.975 | -11.533 | – | -1.737 | 2.196 | 17.5 |
| Cantat-Gaudin et al. (2018) | 106.038 | -11.475 | 0.842 | -4.54 | 1.618 | – |
| Soubiran et al. (2018) | 106.038 | -11.475 | – | – | – | 27.99 |
| Dias et al. (2019) | 105.975 | -11.533 | 0.86 | -4.469 | 1.461 | 25.6 |
| Cantat-Gaudin et al. (2020) | 106.038 | -11.475 | 0.842 | -4.54 | 1.618 | – |
| Dias et al. (2021) | 106.043 | -11.488 | 0.834 | -4.539 | 1.607 | 27.58 |
| Santos-Silva et al. (2021) | 106.11 | -11.45 | 0.85 | -4.2 | 1.52 | – |
| He et al. (2022) | 106.186 | -11.333 | 0.866 | -3.997 | 1.506 | – |
| Hunt & Reffert (2023) | 106.037 | -11.442 | 0.875 | -4.385 | 1.583 | 22.272 |
| Cavallo et al. (2024) | 106.099 | -11.456 | 0.869 | – | – | – |
| Celli et al. (2024) | 106.038 | -11.475 | – | – | – | – |
| Hunt & Reffert (2024) | 106.037 | -11.442 | 0.875 | -4.385 | 1.583 | 22.272 |
| Almeida et al. (2025) | 106.043 | -11.488 | – | – | – | – |
| UCC | 106.049 | -11.481 | 0.864 | -4.409 | 1.565 | 24.517 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.25, Dist=1500.0, Age=7.59 |
| Piskunov et al. (2007) | E(B-V)=0.25, Dist=1500, logt=7.59, logM=2.178 |
| Piskunov et al. (2008) | E(B-V)=0.25, Dist=1500, logt=7.59, logM=2.818, logMA=2.772 |
| Loktin & Popova (2017) | E(B-V)=0.335, Dist=1419, logt=6.79 |
| Cantat-Gaudin et al. (2018) | dmode=1148.6 |
| Soubiran et al. (2018) | dmode=1148.6 |
| Dias et al. (2019) | E(B-V)=0.3, Dist=1085, logAge=6.852, Z=0.034 |
| Cantat-Gaudin et al. (2020) | AVNN=1.27, DistPc=1193.0, AgeNN=6.89 |
| Dias et al. (2021) | Av=0.984, Dist=1114, logage=6.749, [Fe/H]=0.025 |
| Santos-Silva et al. (2021) | AVPM=0.96, AVPf=1.18, DPM=1099, DPf=1069.0, AgeM=10.1, AgeF=9, [Fe/H]M=-0.15, [Fe/H]f=0.07 |
| He et al. (2022) | A0=1.4, logAge=6.75 |
| Hunt & Reffert (2023) | AV50=1.109, diffAV50=2.382, MOD50=10.192, logAge50=6.643 |
| Cavallo et al. (2024) | AV50=1.16, dMod50=10.25, logAge50=6.54, [Fe/H]50=-0.15 |
| Celli et al. (2024) | Age=7.8, Mc=363.3 |
| Hunt & Reffert (2024) | MassJ=735.499, MassTot=735.499 |
| Almeida et al. (2025) | AV=0.984, Dist=1114, logAge=6.749, MassRk=558.6 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWWDL 14341 | 0.3 | 106.46 | -11.12 | 0.85 | -3.92 | 1.46 | 22.47 | 0.12 |