HSC 230

Click to load Aladin Lite
0.09 UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.19
Cdup
Radius (P>50% members) 2.9 [arcmin]
  • CN 0.75 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.19 Likely duplicate

Overview

â„šī¸
HSC 230 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

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

Relatively close High extinction Massive 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 – 277.911 -10.166 0.306 -1.167 -3.326 33.579
Hunt & Reffert 2024 277.924 -10.169 0.311 -1.162 -3.315 46.882
Cavallo et al. 2024 277.982 -10.051 0.311 – – –
Hunt & Reffert 2023 277.924 -10.169 0.311 -1.162 -3.315 46.882

💡 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 – – – – – 1846* – –
Cavallo et al. 2024 2.31 4.90 – 54 -0.030 – – –
Hunt & Reffert 2023 2.84 5.04 2.74 39 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 1641 81.1 277.91 -10.17 0.32 -1.17 -3.31 34.01 0.5

💡 Note: The % column shows the percentage of members that HSC 230 shares with each listed object.

Visualization

â„šī¸