Collinder 365
(NGC 6546; MWSC 2812; OCL 24; ESO 521 29)
0.39
UTI
0.0
CN
0.1
Cdens
0.25
CC3
0.81
Clit
1.0
Cdup
Stellar density (N50/rad)
0.5 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.1 Very loose
- CC3 0.25 Low quality
- Clit 0.81 Well-studied
- Cdup 1.0 Unique
Overview
Collinder 365 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is well-studied in the literature.
(*): The parallax distance estimate (~2.67 kpc) differs significantly from the median photometric distance (~0.94 kpc).
Note: This object shares a very 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 | 271.838 | -23.347 | 0.374 | -0.677 | -2.698 | 18.126 |
| Just et al. | 2023 | 271.866 | -23.326 | â | â | â | â |
| Bica et al. | 2019 | 271.836 | -23.303 | â | â | â | â |
| Loktin & Popova | 2017 | 271.845 | -23.325 | â | 3.23 | -2.515 | -29.4 |
| Kharchenko et al. | 2016 | 271.866 | -23.326 | â | â | â | â |
| Dias et al. | 2014 | 271.842 | -23.297 | â | -1.4 | -0.9 | â |
| Kharchenko et al. | 2013 | 271.875 | -23.325 | â | 0.2 | -1.73 | -29.4 |
| Gozha et al. | 2012 | 271.842 | -23.297 | â | â | â | â |
| Piskunov et al. | 2008 | 271.883 | -23.327 | â | â | â | â |
| Kharchenko et al. | 2007 | 271.84 | -23.3 | â | 0.2 | â | -16.67 |
| Piskunov et al. | 2007 | 271.883 | -23.327 | â | â | â | â |
| van den Bergh | 2006 | 271.9 | -23.333 | â | â | â | â |
| Kharchenko et al. | 2005 | 271.89 | -23.33 | â | -1.3 | 0.3 | -16.67 |
| Kharchenko et al. | 2003 | 271.89 | -23.34 | â | -1.12 | -1.43 | â |
| Dias et al. | 2002 | 271.842 | -23.297 | â | -1.4 | -0.9 | -31.1 |
| Dambis | 1999 | 271.842 | -23.297 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 0.94 | 1.52 | â | 525 | -0.334 | 128 | â | â |
| Just et al. | 2023 | â | â | â | 525 | â | 91 | â | â |
| Loktin & Popova | 2017 | 0.94 | 1.52 | â | 73 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.94 | 1.52 | â | 525 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.94 | 1.52 | â | 525 | -0.334 | â | â | â |
| Gozha et al. | 2012 | 0.94 | â | â | 71 | â | 302 | â | â |
| Piskunov et al. | 2008 | 0.94 | 1.52 | â | 525 | â | 164(1) | â | â |
| Piskunov et al. | 2007 | 0.94 | 1.52 | â | 525 | â | 30 | â | â |
| van den Bergh | 2006 | 0.94 | 1.52 | â | 71 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.94 | 1.52 | â | 525 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.94 | 1.52 | â | â | â | â | â | â |
| Dias et al. | 2002 | 0.94 | 1.52 | â | 71 | -0.334 | â | â | â |
| Dambis | 1999 | 0.86 | 1.68 | â | 126 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA
