HSC 644

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0.20 UTI
0.34
CN
0.14
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.6 [arcmin]
  • CN 0.34 Poorly populated
  • Cdens 0.14 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 644 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a metal-rich, very young 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.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Distant High extinction Metal-rich Very young

Cavallo et al. (2024)
Wood sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 310.454 43.428 0.275 -2.454 -4.192 -44.139
Hunt & Reffert 2024 310.462 43.399 0.296 -2.459 -4.198 –
Cavallo et al. 2024 310.449 43.453 0.288 – – –
Hunt & Reffert 2023 310.462 43.399 0.296 -2.459 -4.198 –

💡 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 – – – – – 799* – –
Cavallo et al. 2024 3.21 4.43 – 20 0.730 – – –
Hunt & Reffert 2023 3.16 5.48 2.48 7 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3888 91.2 310.46 43.45 0.28 -2.45 -4.19 -44.14 0.03

💡 Note: The % column shows the percentage of members that HSC 644 shares with each listed object.

Visualization

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