HSC 226

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0.45 UTI
0.5
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.9 [arcmin]
  • CN 0.5 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 226 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a 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.

Relatively close High extinction Near-solar metallicity Young

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 – 277.618 -10.471 0.464 0.17 -0.047 39.91
Hunt & Reffert 2024 277.621 -10.45 0.467 0.173 -0.066 5.86
Cavallo et al. 2024 277.613 -10.478 0.462 – – –
Hunt & Reffert 2023 277.621 -10.45 0.467 0.173 -0.066 5.86

💡 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 – – – – – 859* – –
Cavallo et al. 2024 1.51 4.45 – 89 -0.210 – – –
Hunt & Reffert 2023 2.01 4.51 1.98 40 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3670 96.1 277.61 -10.47 0.46 0.17 -0.05 39.91 0.06

💡 Note: The % column shows the percentage of members that HSC 226 shares with each listed object.

Visualization

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