HSC 449

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0.37 UTI
0.55
CN
0.29
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.3 [arcmin]
  • CN 0.55 Moderately populated
  • Cdens 0.29 Loose
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 449 is a moderately populated, loose object of very high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by 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 moderate percentage of members with a later reported entry. See table with shared members information.

Distant High extinction Massive 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 – 293.188 19.354 0.195 -2.502 -5.399 25.055
Hunt & Reffert 2024 293.205 19.372 0.198 -2.479 -5.392 31.571
Cavallo et al. 2024 293.187 19.365 0.197 – – –
Hunt & Reffert 2023 293.205 19.372 0.198 -2.479 -5.392 31.571

💡 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 – – – – – 2393* – –
Cavallo et al. 2024 4.79 4.71 – 81 -0.110 – – –
Hunt & Reffert 2023 4.60 4.77 2.60 89 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3766 46.7 293.17 19.3 0.2 -2.54 -5.43 30.3 0.01

💡 Note: The % column shows the percentage of members that HSC 449 shares with each listed object.

Visualization

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