HSC 2304

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0.13 UTI
0.74
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.27
Cdup
Radius (P>50% members) 11.0 [arcmin]
  • CN 0.74 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.27 Possibly duplicate

Overview

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HSC 2304 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a 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.

Relatively close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 147.326 -60.149 0.903 -7.072 4.131 -0.464
Hunt & Reffert 2024 147.315 -60.184 0.899 -7.092 4.119 -4.461
Cavallo et al. 2024 147.358 -60.11 0.901 – – –
Hunt & Reffert 2023 147.315 -60.184 0.899 -7.092 4.119 -4.461

💡 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 – – – – – 182* – –
Cavallo et al. 2024 1.03 0.33 – 355 -0.070 – – –
Hunt & Reffert 2023 1.06 0.20 0.39 187 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 2290 73.2 147.29 -60.14 0.9 -7.07 4.14 -0.37 0.47
CWWDL 14103 70.1 147.36 -60.15 0.9 -7.09 4.13 -0.74 0.03

💡 Note: The % column shows the percentage of members that HSC 2304 shares with each listed object.

Visualization

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