HSC 1633

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0.33 UTI
0.59
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.63
Cdup
Radius (P>50% members) 29.7 [arcmin]
  • CN 0.59 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.63 Likely unique

Overview

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HSC 1633 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Very close Low extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 80.923 -4.497 2.627 1.876 -1.054 21.379
Zhang et al. 2024 80.753 -4.581 – – – –
Cavallo et al. 2024 80.893 -4.41 2.632 – – –
Hunt & Reffert 2023 80.753 -4.581 2.634 1.845 -1.041 14.802

💡 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
Zhang et al. 2024 – – – – -0.072* – – –
Cavallo et al. 2024 0.39 0.87 – 4 -0.220 – – –
Hunt & Reffert 2023 0.37 0.32 0.89 6 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14540 36.8 80.99 -4.51 2.62 1.93 -1.11 3.14 0.35

💡 Note: The % column shows the percentage of members that HSC 1633 shares with each listed object.

Visualization

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