HSC 253

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0.15 UTI
0.0
CN
0.13
Cdens
0.75
CC3
0.0
Clit
0.88
Cdup
Radius (P>50% members) 10.0 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.13 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.88 Very likely unique

Overview

â„šī¸
HSC 253 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.88) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Moderate extinction Metal-rich Young

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 – 279.073 -5.953 0.489 -0.804 -2.255 –
Hunt & Reffert 2024 279.098 -6.0 0.499 -0.801 -2.223 –
Cavallo et al. 2024 279.137 -5.988 0.499 – – –
Hunt & Reffert 2023 279.098 -6.0 0.499 -0.801 -2.223 –

💡 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 – – – – – 163* – –
Cavallo et al. 2024 2.33 2.94 – 34 0.500 – – –
Hunt & Reffert 2023 1.88 2.44 1.50 104 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Ryu 255 12.0 279.3 -5.99 0.45 -0.81 -2.27 116.31 0.28

💡 Note: The % column shows the percentage of members that HSC 253 shares with each listed object.

Visualization

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