Bica 3
(MWSC 2915; BBD 4; FSR 0057)
0.37
UTI
0.0
CN
0.15
Cdens
0.12
CC3
0.78
Clit
1.0
Cdup
Stellar density (N50/rad)
0.8 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.15 Very loose
- CC3 0.12 Very low quality
- Clit 0.78 Well-studied
- Cdup 1.0 Unique
Overview
Bica 3 is a sparse, very loose object of very low 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, very young cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 276.529 | -13.068 | 0.401 | -0.58 | -1.629 | 6.48 |
| Hunt & Reffert | 2024 | 276.517 | -13.06 | 0.332 | -0.177 | -1.681 | 14.936 |
| Celli et al. | 2024 | 276.519 | -13.058 | β | β | β | β |
| Cavallo et al. | 2024 | 276.519 | -13.062 | 0.328 | β | β | β |
| Hunt & Reffert | 2023 | 276.517 | -13.06 | 0.332 | -0.177 | -1.681 | 14.936 |
| Just et al. | 2023 | 276.509 | -13.052 | β | β | β | β |
| Cantat-Gaudin et al. | 2020 | 276.519 | -13.058 | 0.391 | -0.588 | -1.598 | β |
| SΓ‘nchez et al. | 2020 | 276.517 | -13.059 | β | -0.519 | -1.572 | β |
| Cantat-Gaudin & Anders | 2020 | 276.519 | -13.058 | 0.391 | -0.588 | -1.598 | β |
| Bica et al. | 2019 | 276.519 | -13.065 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 276.519 | -13.058 | 0.391 | -0.588 | -1.598 | β |
| Kharchenko et al. | 2016 | 276.509 | -13.052 | β | β | β | β |
| Dias et al. | 2014 | 276.517 | -13.059 | β | 1.71 | 1.07 | β |
| Kharchenko et al. | 2013 | 276.516 | -13.05 | β | -1.33 | -5.15 | β |
| Dias et al. | 2002 | 276.517 | -13.059 | β | 1.8 | 0.95 | β |
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 | 2.38 | 6.76 | 3.09 | 16 | 0.100 | 749 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1647(1) | β | β |
| Celli et al. | 2024 | β | β | β | 16 | β | 749 | β | β |
| Cavallo et al. | 2024 | 3.44 | 5.88 | β | 4 | 0.100 | β | β | β |
| Hunt & Reffert | 2023 | 2.75 | 4.45 | 3.09 | 42 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 16 | β | 56 | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.38 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.38 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 1.61 | 7.10 | β | 16 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.61 | 7.10 | β | 16 | β | β | β | β |
| Dias et al. | 2002 | 1.64 | 6.76 | β | 25 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Wood sample.