HSC 2829

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0.29 UTI
0.4
CN
0.65
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 12.0 [arcmin]
  • CN 0.4 Poorly populated
  • Cdens 0.65 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2829 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
Close Moderate extinction Near-solar metallicity Very 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 – 255.243 -46.227 0.999 -0.639 -2.969 -2.539
Hunt & Reffert 2024 255.253 -46.183 0.991 -0.646 -2.915 8.405
Cavallo et al. 2024 255.228 -46.235 0.994 – – –
Hunt & Reffert 2023 255.253 -46.183 0.991 -0.646 -2.915 8.405

💡 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 – – – – – 186* – –
Cavallo et al. 2024 0.84 2.08 – 19 -0.380 – – –
Hunt & Reffert 2023 0.94 2.04 2.12 17 – – – –

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

Visualization

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