UBC 1601

Click to load Aladin Lite
0.29 UTI
0.0
CN
0.2
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.2 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
UBC 1601 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 319.906 55.074 0.31 -3.694 -3.892 -34.561
Hunt & Reffert 2024 319.926 55.08 0.309 -3.686 -3.872 -34.634
Cavallo et al. 2024 319.9 55.07 0.317 – – –
Hunt & Reffert 2023 319.926 55.08 0.309 -3.686 -3.872 -34.634
Castro-Ginard et al. 2022 319.91 55.06 0.3 -3.69 -3.87 –

💡 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] Bfr BSS
Hunt & Reffert 2024 – – – – – 220* – –
Cavallo et al. 2024 2.64 2.18 – 89 0.250 – – –
Hunt & Reffert 2023 2.88 2.31 1.21 55 – – – –
Castro-Ginard et al. 2022 3.55 1.94 – 102 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 12297 72.0 319.91 55.07 0.3 -3.67 -3.84 – 0.08

💡 Note: The % column shows the percentage of members that UBC 1601 shares with each listed object.

Visualization

â„šī¸