NGC 7438
(FSR 0380; MWSC 3682)
0.54
UTI
0.0
CN
0.22
Cdens
0.75
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
19.1 [arcmin]
- CN 0.0 Sparse
- Cdens 0.22 Very loose
- CC3 0.75 High quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
NGC 7438 is a sparse, very loose object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is well-studied in the literature.
Close
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 344.793 | 54.322 | 1.209 | -2.275 | -4.264 | -34.759 |
| Zhang et al. | 2024 | 344.671 | 54.251 | â | â | â | â |
| Cavallo et al. | 2024 | 345.645 | 54.546 | 1.227 | â | â | â |
| Hunt & Reffert | 2023 | 344.671 | 54.251 | 1.231 | -2.204 | -4.247 | -37.127 |
| Just et al. | 2023 | 344.333 | 54.371 | â | â | â | â |
| Bica et al. | 2019 | 344.327 | 54.357 | â | â | â | â |
| Loktin & Popova | 2017 | 344.34 | 54.339 | â | -0.535 | -0.535 | -17.0 |
| Kharchenko et al. | 2016 | 344.333 | 54.371 | â | â | â | â |
| Dias et al. | 2014 | 344.342 | 54.338 | â | -2.14 | -0.67 | â |
| Kharchenko et al. | 2013 | 344.34 | 54.375 | â | 0.01 | -1.55 | -17.0 |
| Gozha et al. | 2012 | 344.341 | 54.339 | â | â | â | â |
| Kharchenko et al. | 2012 | 344.34 | 54.375 | â | 0.01 | -1.55 | -17.0 |
| Piskunov et al. | 2008 | 344.326 | 54.335 | â | â | â | â |
| Kharchenko et al. | 2007 | 344.34 | 54.34 | â | 0.23 | â | -17.0 |
| Piskunov et al. | 2007 | 344.326 | 54.335 | â | â | â | â |
| Froebrich et al. | 2007 | 344.146 | 54.251 | â | â | â | â |
| Kharchenko et al. | 2005 | 344.34 | 54.34 | â | 1.53 | -1.18 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | 0.005* | â | â | â |
| Cavallo et al. | 2024 | 0.83 | 0.92 | â | 269 | 0.460 | â | â | â |
| Hunt & Reffert | 2023 | 0.77 | 0.81 | 0.32 | 238 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 631 | â | 92 | â | â |
| Loktin & Popova | 2017 | 2.08 | 0.28 | â | 631 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.00 | 1.08 | â | 631 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.00 | 1.08 | â | 631 | â | â | â | â |
| Gozha et al. | 2012 | 0.60 | â | â | 851 | â | 98 | â | â |
| Kharchenko et al. | 2012 | 1.00 | 1.08 | â | 631 | â | â | â | â |
| Piskunov et al. | 2008 | 0.60 | 1.24 | â | 851 | â | 121* | â | â |
| Piskunov et al. | 2007 | 0.60 | 1.24 | â | 851 | â | 22 | â | â |
| Kharchenko et al. | 2005 | 0.60 | 1.24 | â | 851 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.