FSR 0087
(MWSC 2989)
0.74
UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.6
Clit
1.0
Cdup
Stellar density (N50/rad)
15.4 [N/pc2]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0087 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, intermediate-age cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~2.59 kpc) differs significantly from the median photometric distance (~1.17 kpc).
Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 281.413 | -3.614 | 0.386 | -0.217 | -4.252 | 31.34 |
| Hunt & Reffert | 2024 | 281.405 | -3.602 | 0.388 | -0.223 | -4.258 | 48.961 |
| Cavallo et al. | 2024 | 281.396 | -3.628 | 0.387 | â | â | â |
| Hunt & Reffert | 2023 | 281.405 | -3.602 | 0.388 | -0.223 | -4.258 | 48.961 |
| Just et al. | 2023 | 281.476 | -3.608 | â | â | â | â |
| Bica et al. | 2019 | 281.498 | -3.62 | â | â | â | â |
| Kharchenko et al. | 2016 | 281.476 | -3.608 | â | â | â | â |
| Dias et al. | 2014 | 281.5 | -3.621 | â | 1.66 | 0.04 | â |
| Kharchenko et al. | 2013 | 281.482 | -3.607 | â | -0.28 | -6.48 | â |
| Morales et al. | 2013 | 281.5 | -3.621 | â | â | â | â |
| Froebrich et al. | 2007 | 281.5 | -3.621 | â | â | â | â |
| Dias et al. | 2002 | 281.5 | -3.621 | â | 1.66 | 0.04 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.17 | 4.84 | 2.81 | 178 | 0.690 | 1209 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 2313(1) | â | â |
| Cavallo et al. | 2024 | 2.73 | 4.74 | â | 123 | 0.690 | â | â | â |
| Hunt & Reffert | 2023 | 2.35 | 5.37 | 2.81 | 74 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 178 | â | 105 | â | â |
| Kharchenko et al. | 2016 | 1.17 | 4.84 | â | 178 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.17 | 4.84 | â | 178 | â | â | â | â |
| Dias et al. | 2002 | 1.17 | 4.84 | â | 178 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.
Cavallo et al. (2024)
Silver sample.