HSC 284

Click to load Aladin Lite
0.39 UTI
0.31
CN
1.0
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.1 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 284 is a poorly populated, very dense object of intermediate 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.

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

Distant High extinction Massive Near-solar metallicity Young

Cavallo et al. (2024)
Silver sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 280.295 -3.908 0.252 -1.515 -3.945 57.61
Hunt & Reffert 2024 280.303 -3.911 0.253 -1.497 -3.958 57.411
Cavallo et al. 2024 280.294 -3.909 0.255 – – –
Hunt & Reffert 2023 280.303 -3.911 0.253 -1.497 -3.958 57.411

💡 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 – – – – – 1200* – –
Cavallo et al. 2024 4.83 4.60 – 16 0.280 – – –
Hunt & Reffert 2023 3.29 4.65 2.43 115 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3599 100.0 280.3 -3.91 0.25 -1.52 -3.94 57.45 0.19

💡 Note: The % column shows the percentage of members that HSC 284 shares with each listed object.

Visualization

â„šī¸