HSC 1678

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0.30 UTI
0.26
CN
0.26
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.5 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.26 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1678 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a large distance, below 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.

Very 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 – 100.368 -1.25 0.162 -0.656 0.996 26.032
Hu & Soubiran 2025 100.356 -1.248 – – – –
Hunt & Reffert 2024 100.348 -1.253 0.172 -0.642 0.994 26.024
Cavallo et al. 2024 100.356 -1.248 0.166 – – –
Hunt & Reffert 2023 100.348 -1.253 0.172 -0.642 0.994 26.024

💡 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
Hu & Soubiran 2025 – – – – -0.250* – – –
Hunt & Reffert 2024 – – – – – 416* – –
Cavallo et al. 2024 4.51 1.49 – 575 0.140 – – –
Hunt & Reffert 2023 5.59 1.79 0.82 318 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3481 100.0 100.36 -1.25 0.17 -0.65 1.01 26.03 0.06

💡 Note: The % column shows the percentage of members that HSC 1678 shares with each listed object.

Visualization

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