HSC 1379

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0.21 UTI
0.46
CN
0.74
Cdens
0.25
CC3
0.25
Clit
0.54
Cdup
Stellar density (N50/rad) 3.7 [N/pc2]
  • CN 0.46 Poorly populated
  • Cdens 0.74 Moderately dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.54 Likely unique

Overview

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HSC 1379 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a relatively close distance, near 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.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 84.447 31.972 0.596 0.74 -2.689 4.589
Zhang et al. 2024 84.464 31.983 – – – –
Hunt & Reffert 2024 84.464 31.983 0.584 0.747 -2.662 10.467
Cavallo et al. 2024 84.33 31.962 0.587 – – –
Hunt & Reffert 2023 84.464 31.983 0.584 0.747 -2.662 10.467

💡 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] Bfrac BSS
UCC 99999– 1.6 2.18 2.53 38 -0.142 390 – –
Zhang et al. 2024 – – – – -0.144(1) – – –
Hunt & Reffert 2024 – – – – – 390(1) – –
Cavallo et al. 2024 1.59 2.30 – 52 -0.140 – – –
Hunt & Reffert 2023 1.61 2.06 2.53 23 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
AFGL 5157 45.7 84.45 31.99 0.6 0.7 -2.72 4.59 0.32

💡 Note: The % column shows the percentage of members that HSC 1379 shares with each listed object.

Visualization

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