HSC 1905

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0.17 UTI
0.0
CN
0.22
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 12.3 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.22 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1905 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, 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 Low extinction Low mass Near-solar metallicity 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 – 112.503 -23.954 0.806 -3.769 3.99 40.541
Hunt & Reffert 2024 112.514 -23.946 0.816 -3.746 4.018 41.683
Cavallo et al. 2024 112.483 -23.897 0.81 – – –
Hunt & Reffert 2023 112.514 -23.946 0.816 -3.746 4.018 41.683

💡 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 – – – – – 46* – –
Cavallo et al. 2024 1.31 0.32 – 74 0.340 – – –
Hunt & Reffert 2023 1.16 0.21 0.42 65 – – – –

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

Visualization

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