HSC 941

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0.26 UTI
0.32
CN
0.62
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 7.1 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 0.62 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 941 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, 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.

Relatively close 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 – 2.552 61.357 0.644 -1.134 -2.458 3.048
Hunt & Reffert 2024 2.528 61.358 0.649 -1.158 -2.466 3.028
Cavallo et al. 2024 2.48 61.346 0.646 – – –
Hunt & Reffert 2023 2.528 61.358 0.649 -1.158 -2.466 3.028

💡 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
Hunt & Reffert 2024 – – – – – 119* – –
Cavallo et al. 2024 1.47 1.75 – 191 0.400 – – –
Hunt & Reffert 2023 1.46 1.73 0.46 165 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3348 90.6 2.52 61.37 0.65 -1.14 -2.46 3.05 0.02

💡 Note: The % column shows the percentage of members that HSC 941 shares with each listed object.

Visualization

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