HSC 937

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0.29 UTI
0.45
CN
0.23
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.7 [arcmin]
  • CN 0.45 Poorly populated
  • Cdens 0.23 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 937 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Very distant Moderate extinction Metal-rich Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 359.482 63.796 0.172 -1.952 -0.525 -115.394
Hunt & Reffert 2024 359.492 63.792 0.184 -1.946 -0.524 -92.044
Cavallo et al. 2024 359.529 63.803 0.182 – – –
Hunt & Reffert 2023 359.492 63.792 0.184 -1.946 -0.524 -92.044

💡 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 – – – – – 635* – –
Cavallo et al. 2024 5.30 2.26 – 120 0.530 – – –
Hunt & Reffert 2023 4.87 2.16 2.67 126 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3294 55.6 359.49 63.79 0.17 -1.95 -0.53 -115.39 0.0

💡 Note: The % column shows the percentage of members that HSC 937 shares with each listed object.

Visualization

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