HSC 330

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0.35 UTI
0.26
CN
0.23
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 20.2 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.23 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 330 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
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 – 292.088 -2.933 1.228 -0.057 -2.449 -15.005
Zhang et al. 2024 292.28 -3.079 – – – –
Hunt & Reffert 2024 292.28 -3.079 1.229 -0.089 -2.462 -23.266
Cavallo et al. 2024 292.096 -2.915 1.229 – – –
Hunt & Reffert 2023 292.28 -3.079 1.229 -0.089 -2.462 -23.266

💡 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 – – – – 0.039* – – –
Hunt & Reffert 2024 – – – – – 50* – –
Cavallo et al. 2024 0.85 1.25 – 32 0.560 – – –
Hunt & Reffert 2023 0.77 1.04 0.92 47 – – – –

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

Visualization

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