NGC 3293
(FoF 228)
Summary
NGC 3293 is a very rich, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is very well-studied in the literature.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dambis (1999) | 158.953 | -58.217 | – | – | – | – |
| Dias et al. (2002) | 158.963 | -58.23 | – | -7.53 | 3.1 | -12.0 |
| Chen et al. (2003) | 159.06 | -58.229 | – | -7.53 | 3.1 | -13.0 |
| Piskunov et al. (2008) | 158.949 | -58.23 | – | – | – | – |
| Kharchenko et al. (2012) | 158.955 | -58.23 | – | -7.22 | 2.11 | – |
| Loktin & Popova (2017) | 158.955 | -58.23 | – | -7.53 | 3.1 | -11.2 |
| Cantat-Gaudin et al. (2018) | 158.97 | -58.231 | 0.376 | -7.671 | 3.344 | – |
| Soubiran et al. (2018) | 158.97 | -58.231 | – | – | – | -13.16 |
| Dias et al. (2019) | 158.963 | -58.23 | 0.379 | -7.671 | 3.35 | -13.16 |
| Liu & Pang (2019) | 158.947 | -58.22 | 0.381 | -7.534 | 3.317 | – |
| Cantat-Gaudin et al. (2020) | 158.97 | -58.231 | 0.376 | -7.671 | 3.344 | – |
| Dias et al. (2021) | 158.966 | -58.228 | 0.375 | -7.672 | 3.339 | – |
| Rain et al. (2021) | 158.97 | -58.231 | 0.376 | -7.671 | 3.344 | – |
| Jaehnig et al. (2021) | 158.973 | -58.233 | 0.413 | -7.684 | 3.351 | – |
| Hunt & Reffert (2023) | 158.966 | -58.239 | 0.396 | -7.673 | 3.374 | -23.232 |
| Cavallo et al. (2024) | 158.966 | -58.233 | 0.395 | – | – | – |
| Celli et al. (2024) | 158.97 | -58.231 | – | – | – | – |
| Hunt & Reffert (2024) | 158.966 | -58.239 | 0.396 | -7.673 | 3.374 | -23.232 |
| Almeida et al. (2025) | 158.966 | -58.228 | – | – | – | – |
| UCC | 158.967 | -58.233 | 0.392 | -7.664 | 3.362 | -13.169 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dambis (1999) | E_B-V_=0.254, DM0=11.67, log_age_=7.0 |
| Dias et al. (2002) | E(B-V)=0.263, Dist=2327.0, Age=7.014 |
| Chen et al. (2003) | HDis=2327, Age=0.01 |
| Piskunov et al. (2008) | E(B-V)=0.25, Dist=2471, logt=6.94, logMA=2.28 |
| Kharchenko et al. (2012) | e_bv=0.333, distance=2441, log_age=6.75 |
| Loktin & Popova (2017) | E(B-V)=0.252, Dist=2471, logt=6.972 |
| Cantat-Gaudin et al. (2018) | dmode=2470.8 |
| Soubiran et al. (2018) | dmode=2470.8 |
| Dias et al. (2019) | E(B-V)=0.27, Dist=1769, logAge=7.137, Z=0.002 |
| Liu & Pang (2019) | Age=0.015, Z=0.0 |
| Cantat-Gaudin et al. (2020) | AVNN=0.9, DistPc=2710.0, AgeNN=7.01 |
| Dias et al. (2021) | Av=1.009, Dist=2334, logage=7.139, [Fe/H]=0.028 |
| Rain et al. (2021) | E(B-V)=0.26, Dist=2470.8, log(Age)=7.01, NBSS=0 |
| Jaehnig et al. (2021) | dmode=2.424 |
| Hunt & Reffert (2023) | AV50=0.75, diffAV50=1.105, MOD50=11.909, logAge50=7.182 |
| Cavallo et al. (2024) | AV50=0.97, dMod50=11.98, logAge50=7.16, [Fe/H]50=-0.08 |
| Celli et al. (2024) | Age=10.2, Mc=2051.5 |
| Hunt & Reffert (2024) | MassJ=1433.27, MassTot=1433.27 |
| Almeida et al. (2025) | AV=1.009, Dist=2334, logAge=7.139, MassRk=1689.2 |
Search coordinates in Bayestar19