Juchert 11
(MWSC 304; DSH J0347.3+5354; FSR 0651)
0.75
UTI
0.75
CN
1.0
Cdens
0.62
CC3
0.69
Clit
1.0
Cdup
Stellar density (N50/rad)
30.6 [N/pc2]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.62 Intermediate quality
- Clit 0.69 Moderately studied
- Cdup 1.0 Unique
Overview
Juchert 11 is a rich, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is moderately studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 56.835 | 53.914 | 0.308 | 1.542 | -0.393 | -9.982 |
| Hunt & Reffert | 2024 | 56.84 | 53.908 | 0.322 | 1.517 | -0.374 | -9.985 |
| Cavallo et al. | 2024 | 56.815 | 53.926 | 0.321 | â | â | â |
| He et al. | 2023 | 56.843 | 53.914 | 0.225 | 1.555 | -0.362 | -9.98 |
| Hunt & Reffert | 2023 | 56.84 | 53.908 | 0.322 | 1.517 | -0.374 | -9.985 |
| Just et al. | 2023 | 56.824 | 53.901 | â | â | â | â |
| Bica et al. | 2019 | 56.821 | 53.909 | â | â | â | â |
| Loktin & Popova | 2017 | 56.82 | 53.91 | â | -1.296 | -5.85 | â |
| Kharchenko et al. | 2016 | 56.824 | 53.901 | â | â | â | â |
| Kharchenko et al. | 2013 | 56.835 | 53.902 | â | -3.25 | -5.02 | â |
| Kharchenko et al. | 2012 | 56.835 | 53.902 | â | -3.25 | -5.02 | â |
| Kronberger et al. | 2006 | 56.825 | 53.91 | â | â | â | â |
| Dias et al. | 2002 | 56.825 | 53.91 | â | 18.07 | -17.76 | 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 | 3.0 | 5.89 | 2.24 | 794 | 0.160 | 549 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1001(1) | â | â |
| Cavallo et al. | 2024 | 3.55 | 4.86 | â | 661 | 0.160 | â | â | â |
| He et al. | 2023 | 4.17 | 6.40 | â | 398 | â | â | â | â |
| Hunt & Reffert | 2023 | 2.83 | 5.22 | 2.24 | 759 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 794 | â | 97 | â | â |
| Loktin & Popova | 2017 | 3.19 | 4.50 | â | 28 | â | â | â | â |
| Kharchenko et al. | 2016 | 3.00 | 5.89 | â | 794 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.00 | 5.89 | â | 794 | â | â | â | â |
| Kharchenko et al. | 2012 | 3.00 | 5.89 | â | 794 | â | â | â | â |
| Kronberger et al. | 2006 | 3.60 | 5.21 | â | â | â | â | â | â |
| Dias et al. | 2002 | 3.00 | 5.89 | â | 794 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Silver sample.