HSC 1904

Click to load Aladin Lite
0.26 UTI
0.25
CN
0.77
Cdens
0.5
CC3
0.0
Clit
0.84
Cdup
Radius (P>50% members) 2.1 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.77 Dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.84 Very likely unique

Overview

â„šī¸
HSC 1904 is a poorly populated, dense object of intermediate 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, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

Distant Moderate extinction Near-solar metallicity Intermediate age

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 – 116.754 -21.63 0.24 -2.39 3.38 77.467
Hunt & Reffert 2024 116.744 -21.625 0.233 -2.383 3.361 –
Cavallo et al. 2024 116.755 -21.627 0.239 – – –
Hunt & Reffert 2023 116.744 -21.625 0.233 -2.383 3.361 –

💡 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 – – – – – 184* – –
Cavallo et al. 2024 3.27 1.26 – 148 -0.340 – – –
Hunt & Reffert 2023 3.71 0.78 0.80 194 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3081 100.0 116.76 -21.63 0.23 -2.4 3.38 77.47 0.12
CWWDL 10984 16.0 116.77 -21.62 0.27 -2.27 3.14 109.14 0.06

💡 Note: The % column shows the percentage of members that HSC 1904 shares with each listed object.

Visualization

â„šī¸