HSC 399

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0.35 UTI
0.25
CN
1.0
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.1 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 399 is a poorly populated, very dense 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 near-solar metallicity, intermediate-age 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.

Relatively close High extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 287.781 13.871 0.301 -1.958 -4.713 4.316
Hunt & Reffert 2024 287.779 13.87 0.3 -1.976 -4.704 18.01
Cavallo et al. 2024 287.774 13.859 0.303 – – –
Hunt & Reffert 2023 287.779 13.87 0.3 -1.976 -4.704 18.01

💡 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 – – – – – 223* – –
Cavallo et al. 2024 2.70 3.31 – 224 -0.020 – – –
Hunt & Reffert 2023 3.00 2.98 1.10 261 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3260 100.0 287.78 13.87 0.3 -1.96 -4.71 13.57 0.19

💡 Note: The % column shows the percentage of members that HSC 399 shares with each listed object.

Visualization

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