HSC 1375

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0.25 UTI
0.0
CN
0.14
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 11.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.14 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1375 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction 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 – 85.907 33.414 0.621 0.488 -3.063 -141.072
Zhang et al. 2024 85.952 33.288 – – – –
Hunt & Reffert 2024 85.952 33.288 0.619 0.487 -3.054 –
Cavallo et al. 2024 85.895 33.431 0.62 – – –
Hunt & Reffert 2023 85.952 33.288 0.619 0.487 -3.054 –

💡 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 – – – – -0.217* – – –
Hunt & Reffert 2024 – – – – – 67* – –
Cavallo et al. 2024 1.71 1.16 – 68 -0.010 – – –
Hunt & Reffert 2023 1.64 1.05 0.96 103 – – – –

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

Visualization

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