HSC 2338

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

Overview

â„šī¸
HSC 2338 is a sparse, 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 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 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 – 157.009 -57.174 0.259 -7.196 3.857 9.961
Hunt & Reffert 2024 157.01 -57.174 0.248 -7.184 3.885 9.952
Cavallo et al. 2024 157.002 -57.174 0.245 – – –
Hunt & Reffert 2023 157.01 -57.174 0.248 -7.184 3.885 9.952

💡 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 – – – – – 624* – –
Cavallo et al. 2024 4.07 3.61 – 51 0.020 – – –
Hunt & Reffert 2023 3.73 3.63 2.83 59 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3193 100.0 157.01 -57.17 0.24 -7.2 3.89 9.96 0.2

💡 Note: The % column shows the percentage of members that HSC 2338 shares with each listed object.

Visualization

â„šī¸