FSR 0088
(MWSC 3006)
0.88
UTI
1.0
CN
1.0
Cdens
1.0
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
4.1 [arcmin]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0088 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a very massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
Note: This object shares a very small percentage of members with 2 later reported entries. See table with shared members information.
Distant
High extinction
Very massive
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 | 282.667 | -4.163 | 0.245 | -1.588 | -4.133 | 68.962 |
| Hunt & Reffert | 2024 | 282.661 | -4.183 | 0.247 | -1.582 | -4.123 | 91.447 |
| Cavallo et al. | 2024 | 282.666 | -4.151 | 0.245 | â | â | â |
| Hunt & Reffert | 2023 | 282.661 | -4.183 | 0.247 | -1.582 | -4.123 | 91.447 |
| Just et al. | 2023 | 282.651 | -4.19 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 282.667 | -4.158 | 0.233 | -1.589 | -4.126 | â |
| Cantat-Gaudin & Anders | 2020 | 282.667 | -4.158 | 0.233 | -1.589 | -4.126 | â |
| Soubiran et al. | 2018 | 282.667 | -4.158 | â | â | â | 67.65 |
| Bica et al. | 2019 | 282.658 | -4.19 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 282.667 | -4.158 | 0.233 | -1.589 | -4.126 | â |
| Kharchenko et al. | 2016 | 282.651 | -4.19 | â | â | â | â |
| Kharchenko et al. | 2013 | 282.658 | -4.188 | â | -0.73 | -4.61 | â |
| Froebrich et al. | 2007 | 282.658 | -4.188 | 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 | 19009* | â | â |
| Cavallo et al. | 2024 | 4.15 | 4.87 | â | 55 | 0.300 | â | â | â |
| Hunt & Reffert | 2023 | 3.53 | 4.89 | 3.03 | 92 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 313 | â | 948 | â | â |
| Cantat-Gaudin et al. | 2020 | 3.06 | 3.62 | â | 166 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.81 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 3.81 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.81 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.84 | 4.68 | â | 313 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.84 | 4.68 | â | 313 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Silver sample.