FSR 0134
(MWSC 3112)
0.47
UTI
0.75
CN
0.4
Cdens
0.75
CC3
0.23
Clit
1.0
Cdup
Nm (P>50%)
110
Core radius and density
2.8 [pc], 2.0 [pc-2]
- CN 0.75 Rich
- Cdens 0.4 Loose
- CC3 0.75 High quality
- Clit 0.23 Rarely studied
- Cdup 1.0 Unique
đĨ Members
đ Colab
đŦ Bayestar19
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
Overview
FSR 0134 is a rich, loose object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 291.118 | 16.89 | 0.173 | -1.99 | -4.426 | 16.341 |
| Hunt & Reffert | 2024 | 291.129 | 16.886 | 0.191 | -1.98 | -4.434 | 13.532 |
| Cavallo et al. | 2024 | 291.119 | 16.906 | 0.181 | â | â | â |
| He et al. | 2023 | 291.114 | 16.895 | 0.161 | -1.996 | -4.42 | 16.34 |
| Hunt & Reffert | 2023 | 291.129 | 16.886 | 0.191 | -1.98 | -4.434 | 13.532 |
| Bica et al. | 2019 | 291.124 | 16.897 | â | â | â | â |
| Dias et al. | 2014 | 291.125 | 16.892 | â | 1.39 | -7.38 | â |
| Morales et al. | 2013 | 291.127 | 16.892 | â | â | â | â |
| Froebrich et al. | 2007 | 291.125 | 16.892 | â | â | â | â |
| Dias et al. | 2002 | 291.125 | 16.892 | â | 1.42 | -7.25 | 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 | 4.18 | 5.32 | 3.06 | 526 | 0.340 | 3049 | â | â |
| Hunt & Reffert | 2024 | 4.18 | 5.32 | 3.06 | 721 | â | 3049(1) | â | â |
| Cavallo et al. | 2024 | 4.63 | 4.97 | â | 331 | 0.340 | â | â | â |
| He et al. | 2023 | 5.89 | 7.10 | â | 251 | â | â | â | â |
| Hunt & Reffert | 2023 | 4.18 | 5.32 | 3.06 | 721 | â | â | â | â |
| Morales et al. | 2013 | 3.20 | â | â | 794 | â | â | â | â |
| Dias et al. | 2002 | 2.48 | 5.19 | â | 10 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Cavallo et al. (2024)
Wood sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.03 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.03 (50th percentile).
Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.