CWNU 1484

Click to load Aladin Lite
0.01 UTI
0.39
CN
0.34
Cdens
0.5
CC3
0.0
Clit
0.03
Cdup
Stellar density (N50/rad) 1.7 [N/pc2]
  • CN 0.39 Poorly populated
  • Cdens 0.34 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.03 Very likely duplicate

Overview

â„šī¸
CWNU 1484 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-rich, very young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD classes: 0.24 (50th percentile), false positive? (human-assigned).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 47.657 56.817 0.4 0.884 -1.141 –
Hunt & Reffert 2024 47.767 56.892 0.399 0.869 -1.131 –
Cavallo et al. 2024 47.631 56.838 0.403 – – –
Hunt & Reffert 2023 47.767 56.892 0.399 0.869 -1.131 –
He et al. 2023 47.561 56.8 0.409 0.92 -1.203 –

💡 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– 2.35 4.31 2.67 10 0.590 370 – –
Hunt & Reffert 2024 – – – – – 370(1) – –
Cavallo et al. 2024 2.26 3.82 – 15 0.590 – – –
Hunt & Reffert 2023 2.35 4.31 2.67 10 – – – –
He et al. 2023 2.75 4.65 – 5 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
IRAS03064+5638 97.4 47.61 56.8 0.41 0.91 -1.12 -13.95 0.25

💡 Note: The % column shows the percentage of members that CWNU 1484 shares with each listed object.

Visualization

â„šī¸