HSC 1910

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0.23 UTI
0.33
CN
0.09
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 7.3 [arcmin]
  • CN 0.33 Poorly populated
  • Cdens 0.09 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1910 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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.

Distant Moderate extinction Metal-rich 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 – 113.026 -24.2 0.245 -2.027 2.681 –
Hunt & Reffert 2024 113.043 -24.203 0.259 -2.03 2.686 –
Cavallo et al. 2024 113.018 -24.178 0.256 – – –
Hunt & Reffert 2023 113.043 -24.203 0.259 -2.03 2.686 –

💡 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 – – – – – 168* – –
Cavallo et al. 2024 3.65 1.44 – 257 0.750 – – –
Hunt & Reffert 2023 3.34 1.78 1.74 58 – – – –

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

Visualization

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