UBC 1504

Click to load Aladin Lite
0.45 UTI
0.0
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
UBC 1504 is a sparse, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

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

Relatively close Low 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 – 175.39 -59.572 0.415 -7.265 1.222 -27.768
Hunt & Reffert 2024 175.399 -59.564 0.413 -7.249 1.233 -27.783
Cavallo et al. 2024 175.393 -59.562 0.417 – – –
Hunt & Reffert 2023 175.399 -59.564 0.413 -7.249 1.233 -27.783
Castro-Ginard et al. 2022 175.42 -59.56 0.42 -7.25 1.21 –

💡 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 – – – – – 190* – –
Cavallo et al. 2024 2.04 0.66 – 490 -0.010 – – –
Hunt & Reffert 2023 2.19 0.81 0.58 65 – – – –
Castro-Ginard et al. 2022 2.88 0.92 – 33 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 2763 80.0 175.4 -59.57 0.41 -7.25 1.22 -27.77 0.1

💡 Note: The % column shows the percentage of members that UBC 1504 shares with each listed object.

Visualization

â„šī¸