NGC 7235
(MWSC 3595)
0.95
UTI
0.79
CN
0.97
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Nm (P>50%)
219
Core radius and density
1.4 [pc], 4.8 [pc-2]
- CN 0.79 Rich
- Cdens 0.97 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 7235 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, very young cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.
Note: This object shares a moderate percentage of members with 3 later reported entries. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 333.07 | 57.27 | 0.268 | -3.779 | -3.079 | -63.394 |
| Almeida et al. | 2025 | 333.085 | 57.275 | β | β | β | β |
| Hunt & Reffert | 2024 | 333.086 | 57.273 | 0.277 | -3.801 | -3.095 | -61.989 |
| Celli et al. | 2024 | 333.083 | 57.271 | β | β | β | β |
| Cavallo et al. | 2024 | 333.056 | 57.278 | 0.277 | β | β | β |
| He et al. | 2023 | 333.162 | 57.26 | 0.199 | -3.101 | -2.77 | -73.94 |
| Hunt & Reffert | 2023 | 333.086 | 57.273 | 0.277 | -3.801 | -3.095 | -61.989 |
| Almeida et al. | 2023 | 333.084 | 57.274 | β | β | β | β |
| Just et al. | 2023 | 333.084 | 57.261 | β | β | β | β |
| Jaehnig et al. | 2021 | 333.067 | 57.266 | 0.287 | -3.811 | -3.038 | β |
| Rain et al. | 2021 | 333.083 | 57.271 | 0.152 | -2.381 | 2.935 | β |
| Dias et al. | 2021 | 333.085 | 57.275 | 0.259 | -3.718 | -3.035 | β |
| Cantat-Gaudin et al. | 2020 | 333.083 | 57.271 | 0.259 | -3.757 | -3.026 | β |
| SΓ‘nchez et al. | 2020 | 333.104 | 57.27 | β | -3.811 | -3.021 | β |
| Cantat-Gaudin & Anders | 2020 | 333.083 | 57.271 | 0.259 | -3.757 | -3.026 | β |
| Dias et al. | 2019 | 333.104 | 57.27 | 0.262 | -3.777 | -3.066 | -57.12 |
| Bossini et al. | 2019 | 333.083 | 57.271 | β | β | β | β |
| Soubiran et al. | 2018 | 333.083 | 57.271 | β | β | β | -57.12 |
| Cantat-Gaudin et al. | 2018 | 333.083 | 57.271 | 0.259 | -3.757 | -3.026 | β |
| Dias et al. | 2018 | β | β | β | -4.39 | -2.54 | β |
| Loktin & Popova | 2017 | 333.105 | 57.27 | β | -0.688 | 0.028 | -53.7 |
| Sampedro et al. | 2017 | 333.104 | 57.27 | β | -1.28 | -2.47 | β |
| Kharchenko et al. | 2016 | 333.084 | 57.261 | β | β | β | β |
| Dias et al. | 2014 | 333.104 | 57.27 | β | -3.57 | -3.15 | β |
| Kharchenko et al. | 2013 | 333.09 | 57.265 | β | -4.54 | -2.35 | -53.7 |
| Gozha et al. | 2012 | 333.104 | 57.27 | β | β | β | β |
| Kharchenko et al. | 2012 | 333.09 | 57.265 | β | -4.54 | -2.35 | -53.7 |
| Bukowiecki et al. | 2011 | 333.096 | 57.266 | β | β | β | β |
| Piskunov et al. | 2008 | 333.105 | 57.268 | β | β | β | β |
| Kharchenko et al. | 2007 | 333.1 | 57.27 | β | 0.08 | β | -53.7 |
| Ahumada & Lapasset | 2007 | 333.1 | 57.267 | β | β | β | β |
| van den Bergh | 2006 | 333.1 | 57.267 | β | β | β | β |
| Kharchenko et al. | 2005 | 333.1 | 57.27 | β | -2.48 | -1.74 | β |
| Chen et al. | 2003 | 333.084 | 57.284 | β | -4.03 | -2.11 | -52.0 |
| Dias et al. | 2002 | 333.104 | 57.27 | β | -4.03 | -2.11 | -53.71 |
| Dambis | 1999 | 333.104 | 57.27 | β | β | β | β |
| Lynga | 1987 | 333.135 | 57.279 | β | β | β | -52.0 |
| Sulentic et al. | 1973 | 333.147 | 57.274 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999β | 3.33 | 2.77 | 1.2 | 13 | -0.125 | 1552 | 0.45 | 0 |
| Almeida et al. | 2025 | 3.16 | 2.57 | β | 13 | β | 1557 | β | β |
| Hunt & Reffert | 2024 | 3.42 | 2.60 | 1.20 | 15 | β | 1882(1) | β | β |
| Celli et al. | 2024 | β | β | β | 9 | β | 1552 | β | β |
| Cavallo et al. | 2024 | 3.30 | 2.48 | β | 59 | 0.630 | β | β | β |
| He et al. | 2023 | 4.37 | 3.35 | β | 158 | β | β | β | β |
| Hunt & Reffert | 2023 | 3.42 | 2.60 | 1.20 | 15 | β | β | β | β |
| Almeida et al. | 2023 | 3.11 | 2.70 | β | 14 | -0.125 | 1635(1) | 0.45 | β |
| Just et al. | 2023 | β | β | β | 20 | β | 159 | β | β |
| Jaehnig et al. | 2021 | 3.52(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 5.54 | 2.56 | β | 10 | β | β | β | 0 |
| Dias et al. | 2021 | 3.16 | 2.57 | β | 13 | 0.018 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 3.94 | 2.37 | β | 9 | β | β | β | β |
| Kounkel et al. | 2020 | 3.45 | 2.67 | β | 56 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 3.47 | β | β | β | β | β | β | β |
| Dias et al. | 2019 | 3.74 | 2.59 | β | 20 | -0.182 | β | β | β |
| Bossini et al. | 2019 | 4.29 | 2.52 | β | 10 | 0.000 | β | β | β |
| Soubiran et al. | 2018 | 3.47 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 3.47 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 2.82 | 2.90 | β | 13 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.70 | 2.94 | β | 20 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.70 | 2.94 | β | 20 | β | β | β | β |
| Bukowiecki et al. | 2012 | β | β | β | β | β | 1042 | β | β |
| Gozha et al. | 2012 | 3.33 | β | β | 8 | -0.620 | 229 | β | β |
| Kharchenko et al. | 2012 | 2.70 | 2.94 | β | 20 | β | β | β | β |
| Bukowiecki et al. | 2011 | 2.88(1) | 2.30 | β | 28 | β | β | β | β |
| Paunzen et al. | 2010 | β | β | β | β | -0.620 | β | β | β |
| Piskunov et al. | 2008 | 2.82 | 2.93 | β | 6 | β | β | β | β |
| Ahumada & Lapasset | 2007 | β | 2.93 | β | 12 | β | β | β | 0 |
| van den Bergh | 2006 | 2.82 | 2.93 | β | 12 | β | β | β | β |
| Kharchenko et al. | 2005 | 2.82 | 2.93 | β | 6 | β | β | β | β |
| Chen et al. | 2003 | 2.82 | β | β | 10 | β | β | β | β |
| Dias et al. | 2002 | 3.33 | 2.84 | β | 8 | β | β | β | β |
| Dambis | 1999 | 2.62 | 2.96 | β | 10 | β | β | β | β |
| Lynga | 1987 | 3.80 | 2.97 | β | 2 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.2681, e_all=0.0626.
Rain et al. (2021)
This cluster was include in (Dias et al., 2002A&A...389..871D, Cat. B/ocl) however, parameters log(t)=7.006, Av=2.516, [Fe/H]=0.00 were taken from Bossini et al. (2019A&A...623A.108B, Cat. J/A+A/623/A108).