NGC 2071
0.47
UTI
0.3
CN
1.0
Cdens
1.0
CC3
0.03
Clit
1.0
Cdup
Stellar density (N50/rad)
351.5 [N/pc2]
- CN 0.3 Poorly populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.03 Rarely studied
- Cdup 1.0 Unique
đĨ Members
đ Colab
đŦ Bayestar19
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
Overview
NGC 2071 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a very close* distance, below the mid-plane, affected by very high extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 10 years.
(*): The parallax distance estimate (~0.44 kpc) differs significantly from the median photometric distance (~0.68 kpc).
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 | 99999â | 86.783 | 0.311 | 2.29 | -1.005 | -0.999 | â |
| Joshi et al. | 2016 | 86.791 | 0.3 | â | â | â | â |
| Lada & Lada | 2003 | 86.792 | 0.322 | â | â | â | â |
| Bica et al. | 2003 | 86.779 | 0.301 | 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 | 0.675 | 9.85 | â | 4 | â | 60 | â | â |
| Joshi et al. | 2016 | 0.95 | 9.85 | â | 4 | â | â | â | â |
| Lada & Lada | 2003 | 0.40 | â | â | â | â | 60 | â | â |
Bica et al. (2003)
Classified as infrared cluster (IRC).
Lada & Lada (2003)
Embedded cluster within âŧ2 Kpc of the Sun.