HSC 221

Click to load Aladin Lite
0.43 UTI
0.41
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.3 [arcmin]
  • CN 0.41 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 221 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, very young cluster (see Parameters). It was recently reported 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 Very high extinction Massive Near-solar metallicity Very 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 – 277.795 -10.88 0.364 0.004 -1.971 38.491
Hunt & Reffert 2024 277.786 -10.875 0.372 -0.039 -1.975 38.474
Cavallo et al. 2024 277.796 -10.893 0.374 – – –
Hunt & Reffert 2023 277.786 -10.875 0.372 -0.039 -1.975 38.474

💡 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 – – – – – 1676* – –
Cavallo et al. 2024 1.86 5.36 – 15 0.070 – – –
Hunt & Reffert 2023 2.52 5.83 2.58 7 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3751 70.7 277.8 -10.9 0.36 0.03 -1.96 38.49 0.03

💡 Note: The % column shows the percentage of members that HSC 221 shares with each listed object.

Visualization

â„šī¸