HSC 2004

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0.12 UTI
0.0
CN
1.0
Cdens
0.62
CC3
0.0
Clit
0.36
Cdup
Radius (P>50% members) 5.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.36 Possibly duplicate

Overview

â„šī¸
HSC 2004 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a metal-rich, young cluster, but with a large variance across recent sources for the absorption parameter (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.

Relatively close Low extinction Metal-rich Young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 121.134 -31.502 0.882 -4.975 4.971 41.691
Hunt & Reffert 2024 121.156 -31.524 0.879 -5.006 5.032 39.071
Cavallo et al. 2024 120.763 -31.301 0.877 – – –
Hunt & Reffert 2023 121.156 -31.524 0.879 -5.006 5.032 39.071

💡 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 – – – – – 90* – –
Cavallo et al. 2024 1.20 0.00 – 35 0.750 – – –
Hunt & Reffert 2023 1.11 0.70 1.38 18 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Casado 3 64.0 121.13 -31.52 0.85 -4.82 4.85 34.7 0.4

💡 Note: The % column shows the percentage of members that HSC 2004 shares with each listed object.

Visualization

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