HSC 1620

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0.01 UTI
0.51
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.02
Cdup
Radius (P>50% members) 1.9 [arcmin]
  • CN 0.51 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.02 Very likely duplicate

Overview

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HSC 1620 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above 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.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously 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 – 101.086 6.971 0.21 -0.139 -0.543 –
Hunt & Reffert 2024 101.089 6.978 0.204 -0.114 -0.491 59.828
Cavallo et al. 2024 101.129 6.953 0.206 – – –
Hunt & Reffert 2023 101.089 6.978 0.204 -0.114 -0.491 59.828

💡 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 – – – – – 691* – –
Cavallo et al. 2024 4.53 1.43 – 174 0.460 – – –
Hunt & Reffert 2023 4.14 1.48 2.08 166 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3179 100.0 101.09 6.97 0.21 -0.14 -0.55 53.15 0.18
Alessi 65 98.1 101.09 6.97 0.21 -0.14 -0.54 53.15 0.46

💡 Note: The % column shows the percentage of members that HSC 1620 shares with each listed object.

Visualization

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