HSC 1935

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0.38 UTI
0.25
CN
1.0
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.4 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1935 is a poorly populated, very dense 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.

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 – 116.551 -25.598 0.189 -1.68 3.309 –
Hunt & Reffert 2024 116.554 -25.602 0.191 -1.722 3.318 –
Cavallo et al. 2024 116.553 -25.607 0.193 – – –
Hunt & Reffert 2023 116.554 -25.602 0.191 -1.722 3.318 –

💡 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 – – – – – 144* – –
Cavallo et al. 2024 5.04 1.60 – 158 -0.190 – – –
Hunt & Reffert 2023 4.65 0.73 0.49 726 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4033 100.0 116.54 -25.59 0.18 -1.67 3.29 95.04 0.18

💡 Note: The % column shows the percentage of members that HSC 1935 shares with each listed object.

Visualization

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