HSC 1380

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0.49 UTI
0.34
CN
0.61
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.4 [arcmin]
  • CN 0.34 Poorly populated
  • Cdens 0.61 Moderately dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1380 is a poorly populated, moderately dense object of very high C3 quality. Its parallax locates it at a moderate distance, well above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age 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 Intermediate age

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 – 90.76 34.999 0.209 0.532 -1.243 1.102
Zhang et al. 2024 90.767 35.012 – – – –
Hunt & Reffert 2024 90.767 35.012 0.236 0.491 -1.199 10.176
Cavallo et al. 2024 90.772 34.978 0.229 – – –
Hunt & Reffert 2023 90.767 35.012 0.236 0.491 -1.199 10.176

💡 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 – – – – -0.161* – – –
Hunt & Reffert 2024 – – – – – 362* – –
Cavallo et al. 2024 3.66 1.94 – 302 -0.270 – – –
Hunt & Reffert 2023 4.00 1.52 2.49 321 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3177 91.2 90.76 34.99 0.21 0.53 -1.24 1.1 0.09

💡 Note: The % column shows the percentage of members that HSC 1380 shares with each listed object.

Visualization

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