NGC 3293
(MWSC 1826; FoF 228)
0.98
UTI
0.9
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
3.3 [arcmin]
- CN 0.9 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 3293 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a massive, near-solar metallicity, very young cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is very well-studied in the literature.
Relatively close
Low extinction
Massive
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 158.967 | -58.233 | 0.392 | -7.664 | 3.362 | -13.169 |
| Li et al. | 2025 | 158.97 | -58.231 | 0.376 | -7.671 | 3.344 | β |
| Wei et al. | 2025 | 158.955 | -58.238 | 0.388 | -7.539 | 3.319 | β |
| Almeida et al. | 2025 | 158.966 | -58.228 | β | β | β | β |
| Hunt & Reffert | 2024 | 158.966 | -58.239 | 0.396 | -7.673 | 3.374 | -23.232 |
| Celli et al. | 2024 | 158.97 | -58.231 | β | β | β | β |
| Cavallo et al. | 2024 | 158.966 | -58.233 | 0.395 | β | β | β |
| Hunt & Reffert | 2023 | 158.966 | -58.239 | 0.396 | -7.673 | 3.374 | -23.232 |
| Almeida et al. | 2023 | 158.945 | -58.217 | β | β | β | β |
| Just et al. | 2023 | 158.948 | -58.227 | β | β | β | β |
| Jaehnig et al. | 2021 | 158.973 | -58.233 | 0.413 | -7.684 | 3.351 | β |
| Rain et al. | 2021 | 158.97 | -58.231 | 0.376 | -7.671 | 3.344 | β |
| Dias et al. | 2021 | 158.966 | -58.228 | 0.375 | -7.672 | 3.339 | β |
| Cantat-Gaudin et al. | 2020 | 158.97 | -58.231 | 0.376 | -7.671 | 3.344 | β |
| SΓ‘nchez et al. | 2020 | 158.963 | -58.23 | β | -7.634 | 3.363 | β |
| Cantat-Gaudin & Anders | 2020 | 158.97 | -58.231 | 0.376 | -7.671 | 3.344 | β |
| Liu & Pang | 2019 | 158.947 | -58.22 | 0.381 | -7.534 | 3.317 | β |
| Dias et al. | 2019 | 158.963 | -58.23 | 0.379 | -7.671 | 3.35 | -13.16 |
| Soubiran et al. | 2018 | 158.97 | -58.231 | β | β | β | -13.16 |
| Cantat-Gaudin et al. | 2018 | 158.97 | -58.231 | 0.376 | -7.671 | 3.344 | β |
| Loktin & Popova | 2017 | 158.955 | -58.23 | β | -7.53 | 3.1 | -11.2 |
| Kharchenko et al. | 2016 | 158.948 | -58.227 | β | β | β | β |
| Dias et al. | 2014 | 158.962 | -58.23 | β | -6.91 | 0.26 | β |
| Kharchenko et al. | 2013 | 158.955 | -58.23 | β | -7.22 | 2.11 | -11.2 |
| Gozha et al. | 2012 | 158.963 | -58.23 | β | β | β | β |
| Piskunov et al. | 2008 | 158.949 | -58.23 | β | β | β | β |
| Kharchenko et al. | 2007 | 158.95 | -58.23 | β | 0.08 | β | -12.29 |
| van den Bergh | 2006 | 158.953 | -58.217 | β | β | β | β |
| Kharchenko et al. | 2005 | 158.95 | -58.23 | β | -7.64 | 3.08 | -12.29 |
| Kharchenko et al. | 2003 | 158.95 | -58.22 | β | -7.21 | 2.24 | β |
| Chen et al. | 2003 | 159.06 | -58.229 | β | -7.53 | 3.1 | -13.0 |
| Dias et al. | 2002 | 158.963 | -58.23 | β | -7.53 | 3.1 | -12.0 |
| Dambis | 1999 | 158.953 | -58.217 | β | β | β | β |
π‘ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 2.50 | 0.85 | β | 13 | 0.141 | β | β | β |
| Wei et al. | 2025 | 2.55 | 0.95 | β | 15 | 0.000 | 6866 | 0.41 | β |
| Almeida et al. | 2025 | 2.33 | 1.01 | β | 14 | β | 1689 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1433* | β | β |
| Celli et al. | 2024 | β | β | β | 10 | β | 2052 | β | β |
| Cavallo et al. | 2024 | 2.49 | 0.97 | β | 14 | -0.080 | β | β | β |
| Hunt & Reffert | 2023 | 2.41 | 0.75 | 1.10 | 15 | β | β | β | β |
| Almeida et al. | 2023 | 2.28 | 0.95 | β | 14 | 0.017 | 1975* | 0.61 | β |
| Just et al. | 2023 | β | β | β | 6 | β | 234 | β | β |
| Jaehnig et al. | 2021 | 2.42* | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 2.47 | 0.81 | β | 10 | β | β | β | 0 |
| Dias et al. | 2021 | 2.33 | 1.01 | β | 14 | 0.028 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.72 | 0.90 | β | 10 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.47 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 15 | 0.000 | β | β | β |
| Dias et al. | 2019 | 1.77 | 0.84 | β | 14 | -2.028 | β | β | β |
| Soubiran et al. | 2018 | 2.47 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.47 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 2.47 | 0.78 | β | 9 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.44 | 1.03 | β | 6 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.44 | 1.03 | β | 6 | β | β | β | β |
| Gozha et al. | 2012 | 2.33 | β | β | 10 | β | 191 | β | β |
| Piskunov et al. | 2008 | 2.47 | 0.78 | β | 9 | β | β | β | β |
| van den Bergh | 2006 | 2.33 | 0.81 | β | 10 | β | β | β | β |
| Kharchenko et al. | 2005 | 2.47 | 0.78 | β | 9 | β | β | β | β |
| Kharchenko et al. | 2003 | 2.33 | 0.78 | β | β | β | β | β | β |
| Chen et al. | 2003 | 2.33 | β | β | 10 | β | β | β | β |
| Dias et al. | 2002 | 2.33 | 0.82 | β | 10 | β | β | β | β |
| Dambis | 1999 | 2.16 | 0.79 | β | 10 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Gold sample.
Cavallo et al. (2024)
Gold sample.