HSC 407

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0.37 UTI
0.75
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.68
Cdup
Radius (P>50% members) 3.1 [arcmin]
  • CN 0.75 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.68 Likely unique

Overview

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HSC 407 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Distant High extinction Massive Near-solar metallicity Intermediate age

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 – 289.19 14.16 0.214 -2.163 -5.498 46.673
Hunt & Reffert 2024 289.205 14.178 0.203 -2.175 -5.489 36.888
Cavallo et al. 2024 289.186 14.167 0.207 – – –
Hunt & Reffert 2023 289.205 14.178 0.203 -2.175 -5.489 36.888

💡 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 – – – – – 1785* – –
Cavallo et al. 2024 3.85 3.47 – 112 0.010 – – –
Hunt & Reffert 2023 4.29 3.42 2.31 88 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 1692 32.4 289.18 14.15 0.22 -2.15 -5.45 58.43 0.42

💡 Note: The % column shows the percentage of members that HSC 407 shares with each listed object.

Visualization

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