HSC 1014

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0.32 UTI
0.44
CN
0.41
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.5 [arcmin]
  • CN 0.44 Poorly populated
  • Cdens 0.41 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1014 is a poorly populated, 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 near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Distant Moderate extinction Near-solar metallicity Very 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 – 20.2 62.524 0.284 -1.583 -0.165 -29.747
Hunt & Reffert 2024 20.188 62.51 0.294 -1.578 -0.179 –
Cavallo et al. 2024 20.167 62.524 0.294 – – –
Hunt & Reffert 2023 20.188 62.51 0.294 -1.578 -0.179 –

💡 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 – – – – – 599* – –
Cavallo et al. 2024 3.45 2.34 – 9 0.160 – – –
Hunt & Reffert 2023 3.11 2.70 1.90 14 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3577 100.0 20.18 62.52 0.28 -1.58 -0.17 -87.63 0.06

💡 Note: The % column shows the percentage of members that HSC 1014 shares with each listed object.

Visualization

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