HSC 624

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0.49 UTI
0.48
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.98
Cdup
Radius (P>50% members) 4.9 [arcmin]
  • CN 0.48 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.98 Unique

Overview

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HSC 624 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It was recently reported in the literature.

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

Relatively close High extinction Metal-rich Young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 307.284 41.281 0.593 -2.581 -3.671 -103.502
Hunt & Reffert 2024 307.284 41.264 0.598 -2.542 -3.459 7.062
Cavallo et al. 2024 307.276 41.324 0.597 – – –
Hunt & Reffert 2023 307.284 41.264 0.598 -2.542 -3.459 7.062

💡 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 – – – – – 505* – –
Cavallo et al. 2024 1.81 4.36 – 58 0.940 – – –
Hunt & Reffert 2023 1.60 5.08 2.77 15 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2605 2.1 307.5 41.51 0.61 -2.45 -2.96 117.61 0.35

💡 Note: The % column shows the percentage of members that HSC 624 shares with each listed object.

Visualization

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