NGC 7082
(OCL 209; MWSC 3517; FoF 2070)
Summary
NGC 7082 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.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 322.321 | 47.127 | – | -1.9 | -2.32 | -9.1 |
| Chen et al. (2003) | 322.307 | 47.124 | – | – | – | – |
| Piskunov et al. (2007) | 322.244 | 47.125 | – | – | – | – |
| Piskunov et al. (2008) | 322.244 | 47.125 | – | – | – | – |
| Kharchenko et al. (2012) | 322.2 | 47.11 | – | -1.03 | -2.12 | – |
| Loktin & Popova (2017) | 322.32 | 47.127 | – | -1.9 | -2.32 | -9.1 |
| Cantat-Gaudin et al. (2018) | 322.186 | 47.103 | 0.729 | -0.293 | -1.106 | – |
| Bica et al. (2019) | 322.347 | 47.081 | – | – | – | – |
| Soubiran et al. (2018) | 322.186 | 47.103 | – | – | – | -24.85 |
| Liu & Pang (2019) | 322.196 | 47.102 | 0.726 | -0.281 | -1.119 | – |
| Cantat-Gaudin et al. (2020) | 322.186 | 47.103 | 0.729 | -0.293 | -1.106 | – |
| Dias et al. (2021) | 322.18 | 47.099 | 0.732 | -0.297 | -1.1 | -15.075 |
| Rain et al. (2021) | 322.186 | 47.103 | 0.729 | -0.293 | -1.106 | – |
| Jaehnig et al. (2021) | 322.175 | 47.106 | 0.765 | -0.29 | -1.108 | – |
| Tarricq et al. (2022) | 322.128 | 47.107 | 0.732 | -0.3 | -1.181 | – |
| Hunt & Reffert (2023) | 322.165 | 47.101 | 0.729 | -0.291 | -1.184 | -10.947 |
| Cavallo et al. (2024) | 322.182 | 47.098 | 0.729 | – | – | – |
| Hunt & Reffert (2024) | 322.165 | 47.101 | 0.729 | -0.291 | -1.184 | -10.947 |
| Almeida et al. (2025) | 322.18 | 47.099 | – | – | – | – |
| UCC | 322.19 | 47.107 | 0.728 | -0.298 | -1.172 | -11.84 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.237, Dist=1442.0, Age=8.233, [Fe/H]=-0.01 |
| Chen et al. (2003) | E(B-V)=0.237, HDis=1442, Age=0.17, [Fe/H]_1=-0.01 |
| Piskunov et al. (2007) | E(B-V)=0.24, Dist=1442, logt=7.91, logM=2.644 |
| Piskunov et al. (2008) | E(B-V)=0.24, Dist=1442, logt=7.91, logM=3.201, logMA=3.595 |
| Kharchenko et al. (2012) | e_bv=0.239, distance=1300, log_age=8.002, metallicity=-0.01 |
| Loktin & Popova (2017) | E(B-V)=0.237, Dist=1442, logt=8.233 |
| Cantat-Gaudin et al. (2018) | dmode=1319.2 |
| Soubiran et al. (2018) | dmode=1319.2 |
| Liu & Pang (2019) | Age=0.132, Z=-0.25 |
| Cantat-Gaudin et al. (2020) | AVNN=0.79, DistPc=1339.0, AgeNN=7.79 |
| Dias et al. (2021) | Av=1.015, Dist=1277, logage=8.134, [Fe/H]=-0.015 |
| Rain et al. (2021) | E(B-V)=0.23, Dist=1319.2, log(Age)=8.23, NBSS=0 |
| Jaehnig et al. (2021) | dmode=1.309 |
| Tarricq et al. (2022) | Dist=1303, logAgeNN=7.81 |
| Hunt & Reffert (2023) | AV50=0.745, diffAV50=0.569, MOD50=10.572, logAge50=8.166 |
| Cavallo et al. (2024) | AV50=0.72, dMod50=10.61, logAge50=8.46, [Fe/H]50=0.41 |
| Hunt & Reffert (2024) | MassJ=1173.67, MassTot=1173.67 |
| Almeida et al. (2025) | AV=1.015, Dist=1277, logAge=8.134, MassRk=1043.5 |
Search coordinates in Bayestar19