HSC 266

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0.44 UTI
0.61
CN
0.6
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.5 [arcmin]
  • CN 0.61 Moderately populated
  • Cdens 0.6 Moderately dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 266 is a moderately populated, moderately dense object of very high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, 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.

Very distant Very high extinction Massive Near-solar metallicity Young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 280.762 -5.775 0.148 -2.238 -5.263 23.276
Hunt & Reffert 2024 280.789 -5.788 0.142 -2.299 -5.304 17.186
Cavallo et al. 2024 280.772 -5.76 0.143 – – –
Hunt & Reffert 2023 280.789 -5.788 0.142 -2.299 -5.304 17.186

💡 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 – – – – – 3390* – –
Cavallo et al. 2024 4.43 5.17 – 71 0.000 – – –
Hunt & Reffert 2023 6.08 4.98 2.91 108 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4269 88.9 280.75 -5.77 0.16 -2.23 -5.25 23.28 0.18

💡 Note: The % column shows the percentage of members that HSC 266 shares with each listed object.

Visualization

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