HSC 1933

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0.28 UTI
0.28
CN
0.61
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.6 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.61 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1933 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low 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 Low 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 – 116.6 -25.526 0.442 -3.252 3.099 47.81
Hunt & Reffert 2024 116.611 -25.534 0.431 -3.268 3.085 –
Cavallo et al. 2024 116.593 -25.536 0.431 – – –
Hunt & Reffert 2023 116.611 -25.534 0.431 -3.268 3.085 –

💡 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 – – – – – 162* – –
Cavallo et al. 2024 2.14 0.89 – 135 -0.070 – – –
Hunt & Reffert 2023 2.06 0.42 0.47 201 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3662 100.0 116.6 -25.53 0.44 -3.25 3.1 47.81 0.0

💡 Note: The % column shows the percentage of members that HSC 1933 shares with each listed object.

Visualization

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