HSC 1274

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0.37 UTI
0.42
CN
0.29
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.0 [arcmin]
  • CN 0.42 Poorly populated
  • Cdens 0.29 Loose
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1274 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a large* distance, near 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.

(*): The parallax distance estimate (~6.13 kpc) differs significantly from the median photometric distance (~4.66 kpc).

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 – 72.547 43.797 0.163 0.585 -0.193 -43.045
Hu & Soubiran 2025 72.535 43.81 – – – –
Hunt & Reffert 2024 72.548 43.796 0.163 0.584 -0.194 -27.223
Cavallo et al. 2024 72.535 43.81 0.165 – – –
Hunt & Reffert 2023 72.548 43.796 0.163 0.584 -0.194 -27.223

💡 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 – – – – -0.150* – – –
Hunt & Reffert 2024 – – – – – 555* – –
Cavallo et al. 2024 4.31 1.85 – 661 -0.280 – – –
Hunt & Reffert 2023 5.02 1.65 1.41 465 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3087 78.6 72.55 43.8 0.15 0.59 -0.19 -43.04 0.0

💡 Note: The % column shows the percentage of members that HSC 1274 shares with each listed object.

Visualization

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