HSC 1362

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0.29 UTI
0.26
CN
0.45
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.8 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.45 Loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1362 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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 – 86.235 35.486 0.324 1.389 -2.908 -2.204
Zhang et al. 2024 86.269 35.488 – – – –
Hunt & Reffert 2024 86.269 35.488 0.31 1.398 -2.903 -2.28
Cavallo et al. 2024 86.207 35.483 0.304 – – –
Hunt & Reffert 2023 86.269 35.488 0.31 1.398 -2.903 -2.28

💡 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 – – – – -0.079* – – –
Hunt & Reffert 2024 – – – – – 369* – –
Cavallo et al. 2024 3.09 2.62 – 380 0.310 – – –
Hunt & Reffert 2023 2.94 2.60 1.25 163 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2941 100.0 86.22 35.48 0.32 1.44 -2.9 -2.2 0.15

💡 Note: The % column shows the percentage of members that HSC 1362 shares with each listed object.

Visualization

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