NGC 6193
(FoF 2224)
Summary
NGC 6193 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 small percentage of members with 4 later reported entries.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dambis (1999) | 250.333 | -48.763 | – | – | – | – |
| Dias et al. (2002) | 250.333 | -48.763 | – | -1.41 | -3.44 | -33.27 |
| Chen et al. (2003) | 250.353 | -48.789 | – | 0.17 | -4.36 | -24.3 |
| Piskunov et al. (2007) | 250.328 | -48.761 | – | – | – | – |
| Piskunov et al. (2008) | 250.328 | -48.761 | – | – | – | – |
| Kharchenko et al. (2012) | 250.343 | -48.755 | – | -0.85 | -5.0 | – |
| Loktin & Popova (2017) | 250.335 | -48.764 | – | -2.898 | -3.834 | -40.0 |
| Cantat-Gaudin et al. (2018) | 250.319 | -48.777 | 0.812 | 1.278 | -4.111 | – |
| Soubiran et al. (2018) | 250.319 | -48.777 | – | – | – | -15.51 |
| Dias et al. (2019) | 250.333 | -48.763 | 0.823 | 1.401 | -3.967 | -14.539 |
| Liu & Pang (2019) | 250.345 | -48.769 | 0.793 | 1.405 | -3.983 | – |
| Cantat-Gaudin et al. (2020) | 250.319 | -48.777 | 0.812 | 1.278 | -4.111 | – |
| Dias et al. (2021) | 250.297 | -48.793 | 0.803 | 1.293 | -4.066 | -64.534 |
| Rain et al. (2021) | 250.319 | -48.777 | 0.812 | 1.278 | -4.111 | – |
| Jaehnig et al. (2021) | 250.337 | -48.772 | 0.832 | 1.336 | -4.023 | – |
| He et al. (2022) | 250.273 | -48.8 | 0.841 | 1.217 | -4.079 | – |
| Hunt & Reffert (2023) | 250.356 | -48.772 | 0.809 | 1.319 | -4.018 | -33.867 |
| Cavallo et al. (2024) | 250.304 | -48.779 | 0.825 | – | – | – |
| Celli et al. (2024) | 250.319 | -48.777 | – | – | – | – |
| Hunt & Reffert (2024) | 250.356 | -48.772 | 0.809 | 1.319 | -4.018 | -33.867 |
| Almeida et al. (2025) | 250.297 | -48.793 | – | – | – | – |
| UCC | 250.321 | -48.785 | 0.816 | 1.276 | -4.058 | -27.744 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dambis (1999) | E_B-V_=0.475, DM0=10.38, log_age_=6.4 |
| Dias et al. (2002) | E(B-V)=0.475, Dist=1155.0, Age=6.775 |
| Chen et al. (2003) | HDis=1155, Age=0.0 |
| Piskunov et al. (2007) | E(B-V)=0.47, Dist=1155, logt=6.9, logM=1.705 |
| Piskunov et al. (2008) | E(B-V)=0.47, Dist=1155, logt=6.9, logM=2.531, logMA=2.772 |
| Kharchenko et al. (2012) | e_bv=0.562, distance=1158, log_age=6.7 |
| Loktin & Popova (2017) | E(B-V)=0.479, Dist=1153, logt=6.781 |
| Cantat-Gaudin et al. (2018) | dmode=1189.6 |
| Soubiran et al. (2018) | dmode=1189.6 |
| Dias et al. (2019) | E(B-V)=0.51, Dist=1031, logAge=6.791, Z=0.023 |
| Liu & Pang (2019) | Age=0.006, Z=-0.25 |
| Cantat-Gaudin et al. (2020) | AVNN=1.72, DistPc=1264.0, AgeNN=6.71 |
| Dias et al. (2021) | Av=1.584, Dist=1080, logage=6.703, [Fe/H]=0.139 |
| Rain et al. (2021) | E(B-V)=0.47, Dist=1189.6, log(Age)=6.77, NBSS=0 |
| Jaehnig et al. (2021) | dmode=1.2 |
| He et al. (2022) | A0=2.05, logAge=6.3 |
| Hunt & Reffert (2023) | AV50=2.087, diffAV50=2.714, MOD50=10.271, logAge50=6.613 |
| Cavallo et al. (2024) | AV50=1.73, dMod50=10.37, logAge50=6.77, [Fe/H]50=-0.02 |
| Celli et al. (2024) | Age=5.1, Mc=1733.4 |
| Hunt & Reffert (2024) | MassJ=2132.20, MassTot=2132.20 |
| Almeida et al. (2025) | AV=1.584, Dist=1080, logAge=6.703, MassRk=1501.7 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 1643 | 14.0 | 250.31 | -48.97 | 0.84 | 0.8 | -4.53 | -28.04 | 0.24 |
| VVV 084 | 2.3 | 250.34 | -48.97 | 0.82 | 1.02 | -4.38 | -37.33 | 0.0 |
| VVV 083 | 2.1 | 250.31 | -49.01 | 0.85 | 0.84 | -4.37 | -27.3 | 0.02 |
| CWNU 1268 | 0.1 | 250.64 | -49.05 | 0.88 | 0.42 | -4.74 | -21.24 | 0.32 |