FSR 0508
(SAI 9; MWSC 66)
0.78
UTI
0.56
CN
1.0
Cdens
0.75
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
1.6 [arcmin]
- CN 0.56 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0508 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by high extinction. It is catalogued as a metal-poor, old cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 10.479 | 64.963 | 0.194 | -2.329 | -0.591 | -118.167 |
| Hunt & Reffert | 2024 | 10.47 | 64.957 | 0.187 | -2.332 | -0.618 | -117.346 |
| Cavallo et al. | 2024 | 10.487 | 64.969 | 0.186 | β | β | β |
| He et al. | 2023 | 10.474 | 64.964 | 0.162 | -2.323 | -0.64 | -118.17 |
| Hunt & Reffert | 2023 | 10.47 | 64.957 | 0.187 | -2.332 | -0.618 | -117.346 |
| Just et al. | 2023 | 10.463 | 64.953 | β | β | β | β |
| SΓ‘nchez et al. | 2020 | 10.492 | 64.981 | β | -2.405 | -0.853 | β |
| Bica et al. | 2019 | 10.468 | 64.983 | β | β | β | β |
| Kharchenko et al. | 2016 | 10.463 | 64.953 | β | β | β | β |
| Dias et al. | 2014 | 10.492 | 64.981 | β | -0.68 | 0.05 | β |
| Kharchenko et al. | 2013 | 10.473 | 64.956 | β | 2.23 | -0.07 | β |
| Kharchenko et al. | 2012 | 10.473 | 64.956 | β | 1.72 | -0.47 | β |
| Glushkova et al. | 2010 | 10.466 | 64.981 | β | β | β | β |
| Froebrich et al. | 2007 | 10.492 | 64.981 | β | β | β | β |
| Dias et al. | 2002 | 10.492 | 64.981 | β | 1.72 | -0.47 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999β | 5.275 | 3.72 | 2.55 | 1072 | -0.610 | 522 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 969(1) | β | β |
| Cavallo et al. | 2024 | 4.90 | 4.00 | β | 1072 | -0.610 | β | β | β |
| He et al. | 2023 | 5.75 | 3.60 | β | 1585 | β | β | β | β |
| Hunt & Reffert | 2023 | 4.38 | 3.48 | 2.55 | 575 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 5 | β | 76 | β | β |
| Kharchenko et al. | 2016 | 5.05 | 4.65 | β | 5 | β | β | β | β |
| Kharchenko et al. | 2013 | 5.05 | 4.65 | β | 5 | β | β | β | β |
| Kharchenko et al. | 2012 | 5.50 | 3.72 | β | 1514 | β | β | β | β |
| Glushkova et al. | 2010 | 7.70 | 2.05 | β | 1259 | β | β | β | β |
| Dias et al. | 2002 | 5.50 | 3.72 | β | 1514 | β | β | β | β |
(N): Indicates that are N extra values assigned to this parameter in the corresponding reference.


Cavallo et al. (2024)
Silver sample.