NGC 2175
0.78
UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
7.0 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
NGC 2175 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is moderately studied in the literature.
Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.
Relatively close
Moderate extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 92.404 | 20.597 | 0.501 | 0.289 | -2.263 | 23.039 |
| Hunt & Reffert | 2024 | 92.349 | 20.636 | 0.512 | 0.386 | -2.246 | 23.043 |
| Cavallo et al. | 2024 | 92.51 | 20.556 | 0.517 | â | â | â |
| Hunt & Reffert | 2023 | 92.349 | 20.636 | 0.512 | 0.386 | -2.246 | 23.043 |
| Jaehnig et al. | 2021 | 92.433 | 20.562 | 0.513 | 0.419 | -2.33 | â |
| Loktin & Popova | 2017 | 92.415 | 20.487 | â | 0.382 | -2.656 | 22.0 |
| Dias et al. | 2014 | 92.412 | 20.487 | â | 0.37 | -5.39 | â |
| Gozha et al. | 2012 | 92.413 | 20.487 | â | â | â | â |
| Kharchenko et al. | 2007 | 92.41 | 20.49 | â | 0.18 | â | â |
| van den Bergh | 2006 | 92.425 | 20.5 | â | â | â | â |
| Chen et al. | 2003 | 92.417 | 20.309 | â | 1.8 | -2.26 | 22.0 |
| Dias et al. | 2002 | 92.412 | 20.487 | â | 1.8 | -2.26 | 23.2 |
| Dambis | 1999 | 92.412 | 20.487 | â | â | â | â |
đĄ 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 229* | â | â |
| Cavallo et al. | 2024 | 1.78 | 1.73 | â | 7 | -0.300 | â | â | â |
| Hunt & Reffert | 2023 | 1.79 | 1.49 | 1.89 | 6 | â | â | â | â |
| Jaehnig et al. | 2021 | 2.00* | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.62 | 1.82 | â | 9 | â | â | â | â |
| Gozha et al. | 2012 | 1.63 | â | â | 9 | â | â | â | â |
| van den Bergh | 2006 | 1.63 | 1.86 | â | 9 | â | â | â | â |
| Chen et al. | 2003 | 1.63 | â | â | 0 | â | â | â | â |
| Dias et al. | 2002 | 1.63 | 1.85 | â | 9 | â | â | â | â |
| Dambis | 1999 | 1.79 | 2.41 | â | 3 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Silver sample.