HSC 1595

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0.23 UTI
0.0
CN
0.14
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.14 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1595 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, 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 Low extinction Near-solar metallicity Intermediate age

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 – 100.717 12.489 0.209 -0.021 -0.483 –
Zhang et al. 2024 100.744 12.511 – – – –
Hunt & Reffert 2024 100.744 12.511 0.189 0.032 -0.545 49.95
Cavallo et al. 2024 100.717 12.501 0.196 – – –
Hunt & Reffert 2023 100.744 12.511 0.189 0.032 -0.545 49.95

💡 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
Zhang et al. 2024 – – – – -0.183* – – –
Hunt & Reffert 2024 – – – – – 193* – –
Cavallo et al. 2024 4.49 1.03 – 186 -0.060 – – –
Hunt & Reffert 2023 4.00 0.90 1.81 187 – – – –

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

Visualization

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