HSC 408

Click to load Aladin Lite
0.33 UTI
0.44
CN
0.48
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.5 [arcmin]
  • CN 0.44 Poorly populated
  • Cdens 0.48 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 408 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a large distance, above 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)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 289.565 14.455 0.17 -1.492 -3.99 31.125
Hunt & Reffert 2024 289.568 14.457 0.182 -1.497 -3.995 44.767
Cavallo et al. 2024 289.564 14.465 0.184 – – –
Hunt & Reffert 2023 289.568 14.457 0.182 -1.497 -3.995 44.767

💡 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 – – – – – 1225* – –
Cavallo et al. 2024 4.37 4.56 – 71 -0.260 – – –
Hunt & Reffert 2023 4.98 4.43 2.52 38 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3373 100.0 289.56 14.46 0.17 -1.49 -4.0 31.13 0.05

💡 Note: The % column shows the percentage of members that HSC 408 shares with each listed object.

Visualization

â„šī¸