HSC 1130

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0.18 UTI
0.0
CN
0.17
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 7.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.17 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1130 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.

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 Moderate extinction Metal-rich Young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 47.131 58.464 0.423 0.754 -0.961 –
Hunt & Reffert 2024 47.284 58.547 0.414 0.76 -0.917 -22.139
Cavallo et al. 2024 47.044 58.448 0.417 – – –
Hunt & Reffert 2023 47.284 58.547 0.414 0.76 -0.917 -22.139

💡 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 – – – – – 348* – –
Cavallo et al. 2024 2.26 2.63 – 43 0.880 – – –
Hunt & Reffert 2023 2.24 3.05 2.65 10 – – – –

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

Visualization

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