ESO 521 38
(MWSC 2825)
0.78
UTI
0.52
CN
1.0
Cdens
1.0
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
7.7 [arcmin]
- CN 0.52 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
ESO 521 38 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Relatively close
Low 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 | β | 272.397 | -24.544 | 0.816 | 0.381 | -2.413 | -14.889 |
| Hunt & Reffert | 2024 | 272.399 | -24.543 | 0.807 | 0.376 | -2.404 | -8.834 |
| Cavallo et al. | 2024 | 272.38 | -24.573 | 0.808 | β | β | β |
| Hunt & Reffert | 2023 | 272.399 | -24.543 | 0.807 | 0.376 | -2.404 | -8.834 |
| Just et al. | 2023 | 272.332 | -24.531 | β | β | β | β |
| SΓ‘nchez et al. | 2020 | 272.354 | -24.53 | β | -0.132 | -2.104 | β |
| Bica et al. | 2019 | 272.342 | -24.53 | β | β | β | β |
| Kharchenko et al. | 2016 | 272.332 | -24.531 | β | β | β | β |
| Dias et al. | 2014 | 272.354 | -24.53 | β | 1.77 | -2.47 | β |
| Kharchenko et al. | 2013 | 272.34 | -24.53 | β | -0.85 | -2.46 | β |
| Piskunov et al. | 2008 | 272.342 | -24.53 | β | β | β | β |
| Kharchenko et al. | 2005 | 272.35 | -24.53 | β | 0.41 | -2.07 | β |
| Dias et al. | 2002 | 272.354 | -24.53 | β | 1.77 | -2.47 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | β | β | β | β | β | 404* | β | β |
| Cavallo et al. | 2024 | 1.10 | 1.24 | β | 132 | -0.140 | β | β | β |
| Hunt & Reffert | 2023 | 1.19 | 0.83 | 0.88 | 208 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 248 | β | 22 | β | β |
| Kharchenko et al. | 2016 | 1.49 | 1.29 | β | 248 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.49 | 1.29 | β | 248 | β | β | β | β |
| Piskunov et al. | 2008 | 1.80 | 0.68 | β | 126 | β | β | β | β |
| Kharchenko et al. | 2005 | 1.80 | 0.68 | β | 126 | β | β | β | β |
| Dias et al. | 2002 | 1.80 | 0.68 | β | 126 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.