HSC 2305

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0.16 UTI
0.0
CN
0.07
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 10.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.07 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2305 is a sparse, very loose 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 metal-rich, very 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.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close High extinction Metal-rich Very 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 – 153.194 -56.474 0.38 -7.83 4.41 22.716
Hunt & Reffert 2024 153.082 -56.483 0.378 -7.801 4.385 -50.895
Cavallo et al. 2024 153.346 -56.498 0.379 – – –
Hunt & Reffert 2023 153.082 -56.483 0.378 -7.801 4.385 -50.895

💡 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 – – – – – 233* – –
Cavallo et al. 2024 3.18 3.87 – 12 0.740 – – –
Hunt & Reffert 2023 2.42 4.21 2.64 5 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4182 92.0 153.31 -56.47 0.38 -7.82 4.42 -51.09 0.06

💡 Note: The % column shows the percentage of members that HSC 2305 shares with each listed object.

Visualization

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