HSC 1690

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0.46 UTI
0.54
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.5 [arcmin]
  • CN 0.54 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1690 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below 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 – 101.661 -2.097 0.215 -0.346 -0.269 83.286
Hunt & Reffert 2024 101.658 -2.093 0.208 -0.353 -0.272 86.756
Cavallo et al. 2024 101.658 -2.097 0.21 – – –
Hunt & Reffert 2023 101.658 -2.093 0.208 -0.353 -0.272 86.756

💡 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 – – – – – 672* – –
Cavallo et al. 2024 4.43 2.87 – 447 -0.170 – – –
Hunt & Reffert 2023 4.33 2.70 1.77 450 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3096 84.2 101.66 -2.1 0.21 -0.31 -0.3 83.29 0.03

💡 Note: The % column shows the percentage of members that HSC 1690 shares with each listed object.

Visualization

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