HSC 2833

Click to load Aladin Lite
0.19 UTI
0.81
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.36
Cdup
Radius (P>50% members) 3.5 [arcmin]
  • CN 0.81 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.36 Possibly duplicate

Overview

â„šī¸
HSC 2833 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, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Distant High extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Bronze sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 252.993 -44.225 0.348 -1.321 -1.176 -63.644
Hunt & Reffert 2024 252.994 -44.221 0.354 -1.336 -1.213 -53.301
Cavallo et al. 2024 252.986 -44.222 0.351 – – –
Hunt & Reffert 2023 252.994 -44.221 0.354 -1.336 -1.213 -53.301

💡 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 – – – – – 2695* – –
Cavallo et al. 2024 3.60 4.78 – 145 0.220 – – –
Hunt & Reffert 2023 2.54 3.66 2.95 429 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 1620 63.9 252.99 -44.23 0.34 -1.32 -1.17 -64.5 0.56

💡 Note: The % column shows the percentage of members that HSC 2833 shares with each listed object.

Visualization

â„šī¸