HSC 1648

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0.00 UTI
0.54
CN
0.63
Cdens
1.0
CC3
0.0
Clit
0.0
Cdup
Stellar density (N50/rad) 3.1 [N/pc2]
  • CN 0.54 Moderately populated
  • Cdens 0.63 Moderately dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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HSC 1648 is a moderately populated, moderately 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.

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.

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 99999– 78.952 -6.617 3.46 1.771 -2.93 11.548
Cavallo et al. 2024 78.532 -7.037 3.493 – – –
Hunt & Reffert 2023 77.275 -8.816 3.493 1.737 -2.975 12.161

💡 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] Bfrac BSS
UCC 99999– 0.285 0.49 0.65 8 -0.040 – – –
Cavallo et al. 2024 0.28 0.71 – 6 -0.040 – – –
Hunt & Reffert 2023 0.29 0.27 0.65 11 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 67 100.0 78.63 -6.76 3.49 1.77 -2.97 13.69 0.46

💡 Note: The % column shows the percentage of members that HSC 1648 shares with each listed object.

Visualization

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