Collinder 35
(NGC 1193; FSR 0649; MWSC 256; OCL 390)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
54.5 [N/pc2]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Collinder 35 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a large distance, well below the mid-plane, affected by low extinction. It is catalogued as a massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity and mass parameters (see Parameters). It is very well-studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 46.488 | 44.382 | 0.184 | -0.193 | -0.426 | -81.892 |
| Li et al. | 2025 | 46.486 | 44.383 | 0.159 | -0.125 | -0.329 | β |
| Hu & Soubiran | 2025 | 46.487 | 44.382 | β | β | β | β |
| Almeida et al. | 2025 | 46.484 | 44.383 | β | β | β | β |
| Hunt & Reffert | 2024 | 46.486 | 44.382 | 0.169 | -0.22 | -0.426 | -83.035 |
| Cavallo et al. | 2024 | 46.487 | 44.382 | 0.168 | β | β | β |
| Hunt & Reffert | 2023 | 46.486 | 44.382 | 0.169 | -0.22 | -0.426 | -83.035 |
| Just et al. | 2023 | 46.459 | 44.378 | β | β | β | β |
| Jaehnig et al. | 2021 | 46.489 | 44.385 | 0.171 | -0.161 | -0.328 | β |
| Rain et al. | 2021 | 46.486 | 44.383 | 0.159 | -0.125 | -0.329 | β |
| Dias et al. | 2021 | 46.484 | 44.383 | 0.175 | -0.123 | -0.354 | β |
| Cantat-Gaudin et al. | 2020 | 46.486 | 44.383 | 0.159 | -0.125 | -0.329 | β |
| SΓ‘nchez et al. | 2020 | 46.483 | 44.383 | β | -0.023 | -0.398 | β |
| Donor et al. | 2020 | 46.47 | 44.38 | β | -0.22 | -0.36 | -84.7 |
| Cantat-Gaudin & Anders | 2020 | 46.486 | 44.383 | 0.159 | -0.125 | -0.329 | β |
| Soubiran et al. | 2018 | 46.486 | 44.383 | β | β | β | -83.24 |
| Bica et al. | 2019 | 46.494 | 44.382 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 46.486 | 44.383 | 0.159 | -0.125 | -0.329 | β |
| Kharchenko et al. | 2016 | 46.459 | 44.378 | β | β | β | β |
| Dias et al. | 2014 | 46.483 | 44.383 | β | 1.05 | -4.96 | β |
| Kharchenko et al. | 2013 | 46.47 | 44.38 | β | -1.47 | 0.42 | -82.0 |
| Gozha et al. | 2012 | 46.483 | 44.383 | β | β | β | β |
| Kharchenko et al. | 2012 | 46.47 | 44.38 | β | -1.47 | 0.42 | -82.0 |
| Kharchenko et al. | 2007 | 46.48 | 44.38 | β | 0.03 | β | β |
| Froebrich et al. | 2007 | 46.504 | 44.387 | β | β | β | β |
| van den Bergh | 2006 | 46.383 | 44.383 | β | β | β | β |
| Chen et al. | 2003 | 46.379 | 44.396 | β | β | β | β |
| Dias et al. | 2002 | 46.483 | 44.383 | β | 1.05 | -4.96 | -82.0 |
π‘ 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 | 99999β | 5.31 | 0.62 | 1.32 | 4571 | -0.293 | 1745 | β | 12.0 |
| Li et al. | 2025 | 5.01 | 0.69 | β | 5279 | -0.314 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.350(5) | β | β | β |
| Almeida et al. | 2025 | 5.52 | 0.70 | β | 4571 | β | 3067 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1745(1) | β | β |
| Cavallo et al. | 2024 | 3.56 | 0.98 | β | 3981 | -0.570 | β | β | β |
| Hunt & Reffert | 2023 | 5.40 | 0.36 | 1.32 | 2183 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 1995 | β | 333 | β | β |
| Jaehnig et al. | 2021 | 6.00(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 5.31 | 0.59 | β | 5012 | β | β | β | 12 |
| Dias et al. | 2021 | 5.52 | 0.70 | β | 4571 | -0.257 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 4.99 | 0.41 | β | 5129 | β | β | β | β |
| Donor et al. | 2020 | β | β | β | β | -0.340 | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 5.31 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 5.31 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 5.31 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 6.00 | 0.62 | β | 1995 | β | β | β | β |
| Kharchenko et al. | 2013 | 6.00 | 0.62 | β | 1995 | -0.293 | β | β | β |
| Gozha et al. | 2012 | 4.57 | β | β | 5012 | -0.220 | β | β | β |
| Kharchenko et al. | 2012 | 6.00 | 0.62 | β | 1995 | -0.293 | β | β | β |
| van den Bergh | 2006 | 4.30 | 0.37 | β | 7943 | β | β | β | β |
| Chen et al. | 2003 | 4.30 | 0.37 | β | 7900 | -0.290(1) | β | β | β |
| Dias et al. | 2002 | 4.57 | 0.59 | β | 5012 | -0.293 | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.