Negueruela 1
(MWSC 3757)
0.60
UTI
0.5
CN
0.44
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Nm (P>50%)
50
Core radius and density
1.9 [pc], 2.2 [pc-2]
- CN 0.5 Moderately populated
- Cdens 0.44 Loose
- CC3 0.75 High quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
Negueruela 1 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is moderately studied in the literature.
Note: This object shares a large percentage of members with at least one entry reported in the same catalogue. 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 | 99999β | 356.861 | 63.212 | 0.308 | -2.973 | -1.381 | β |
| Almeida et al. | 2025 | 356.854 | 63.22 | β | β | β | β |
| Hunt & Reffert | 2024 | 356.851 | 63.222 | 0.31 | -2.99 | -1.417 | β |
| Celli et al. | 2024 | 356.849 | 63.219 | β | β | β | β |
| Cavallo et al. | 2024 | 356.851 | 63.213 | 0.31 | β | β | β |
| Hunt & Reffert | 2023 | 356.851 | 63.222 | 0.31 | -2.99 | -1.417 | β |
| Just et al. | 2023 | 356.82 | 63.216 | β | β | β | β |
| Dias et al. | 2021 | 356.854 | 63.22 | 0.291 | -3.023 | -1.333 | β |
| Spina et al. | 2021 | 356.854 | 63.218 | 0.286 | -2.969 | -1.337 | β |
| Cantat-Gaudin et al. | 2020 | 356.849 | 63.219 | 0.289 | -2.988 | -1.343 | β |
| SΓ‘nchez et al. | 2020 | 356.833 | 63.22 | β | -2.911 | -1.367 | β |
| Cantat-Gaudin & Anders | 2020 | 356.849 | 63.219 | 0.289 | -2.988 | -1.343 | β |
| Dias et al. | 2019 | 356.85 | 63.218 | 0.289 | -2.988 | -1.343 | -5.02 |
| Soubiran et al. | 2018 | 356.849 | 63.219 | β | β | β | -5.02 |
| Cantat-Gaudin et al. | 2018 | 356.849 | 63.219 | 0.289 | -2.988 | -1.343 | β |
| Loktin & Popova | 2017 | 356.835 | 63.22 | β | 2.21 | -7.34 | -60.3 |
| Kharchenko et al. | 2016 | 356.82 | 63.216 | β | β | β | β |
| Kharchenko et al. | 2013 | 356.827 | 63.22 | β | 2.15 | -6.98 | -60.3 |
| Kharchenko et al. | 2012 | 356.827 | 63.22 | β | 2.15 | -6.98 | -60.3 |
| Bukowiecki et al. | 2011 | 356.863 | 63.212 | β | β | β | β |
| Dias et al. | 2002 | 356.833 | 63.22 | β | 2.15 | -6.98 | -60.3 |
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 | 2.84 | 3.85 | 1.43 | 10 | -0.224 | 422 | β | β |
| Almeida et al. | 2025 | 2.65 | 3.27 | β | 8 | β | 409 | β | β |
| Hunt & Reffert | 2024 | 4.11 | 3.85 | 1.43 | 4 | β | 467(1) | β | β |
| Celli et al. | 2024 | β | β | β | 17 | β | 422 | β | β |
| Cavallo et al. | 2024 | 3.18 | 3.90 | β | 10 | -0.660 | β | β | β |
| Hunt & Reffert | 2023 | 4.11 | 3.85 | 1.43 | 4 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 10 | β | 571 | β | β |
| Dias et al. | 2021 | 2.65 | 3.27 | β | 8 | -0.224 | β | β | β |
| Spina et al. | 2021 | 3.42 | β | β | 17 | β | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.88 | 3.39 | β | 17 | β | β | β | β |
| Kounkel et al. | 2020 | 2.77 | 3.87 | β | 14 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 3.14 | β | β | β | β | β | β | β |
| Dias et al. | 2019 | 5.69 | 2.90 | β | 7 | 0.374 | β | β | β |
| Soubiran et al. | 2018 | 3.14 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 3.14 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.01 | 3.44 | β | 15 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.80 | 3.94 | β | 10 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.80 | 3.94 | β | 10 | β | β | β | β |
| Bukowiecki et al. | 2012 | β | β | β | β | β | 212 | β | β |
| Kharchenko et al. | 2012 | 2.80 | 3.94 | β | 10 | β | β | β | β |
| Bukowiecki et al. | 2011 | 1.97(1) | 3.00 | β | 45 | β | β | β | β |
| Dias et al. | 2002 | 2.80 | 3.94 | β | 10 | β | 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.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.1932, e_all=0.0838.
Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010). Asterisms and cluster alikes by B. Alessi reported in DAML02.