HSC 660

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0.33 UTI
0.4
CN
1.0
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.6 [arcmin]
  • CN 0.4 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 660 is a poorly populated, very dense object of low 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, young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Distant High extinction Metal-rich 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 – 310.898 44.916 0.31 -3.089 -4.826 –
Hunt & Reffert 2024 310.902 44.918 0.304 -3.092 -4.807 –
Cavallo et al. 2024 310.711 44.859 0.304 – – –
Hunt & Reffert 2023 310.902 44.918 0.304 -3.092 -4.807 –

💡 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 – – – – – 580* – –
Cavallo et al. 2024 3.82 3.34 – 112 0.790 – – –
Hunt & Reffert 2023 2.87 4.31 3.16 27 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3371 57.5 310.9 44.91 0.32 -3.09 -4.88 – 0.02

💡 Note: The % column shows the percentage of members that HSC 660 shares with each listed object.

Visualization

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