CWNU 1007

Click to load Aladin Lite
0.41 UTI
0.32
CN
0.75
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 3.7 [N/pc2]
  • CN 0.32 Poorly populated
  • Cdens 0.75 Dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1007 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 79.329 18.525 2.794 0.035 -5.749 19.168
Zhang et al. 2024 79.208 18.478 – – – –
Cavallo et al. 2024 80.71 17.076 2.774 – – –
Hunt & Reffert 2023 79.208 18.478 2.774 -0.267 -5.641 23.588
He et al. 2022 79.355 18.504 2.866 -0.099 -5.895 –

💡 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 99999– 0.365 0.96 0.58 19 0.014 – – –
Zhang et al. 2024 – – – – -0.072(1) – – –
Cavallo et al. 2024 0.38 0.96 – 11 0.100 – – –
Hunt & Reffert 2023 0.35 0.58 0.58 19 – – – –
He et al. 2022 – 1.25 – 35 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 111 100.0 79.29 18.61 2.83 -0.11 -5.87 21.26 0.46
LISC-III 3645 59.4 79.51 18.09 2.72 0.1 -5.64 24.35 0.0

💡 Note: The % column shows the percentage of members that CWNU 1007 shares with each listed object.

Visualization

â„šī¸