HSC 2411

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0.25 UTI
0.25
CN
0.64
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.7 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.64 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2411 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 low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Low extinction Near-solar metallicity Intermediate age

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 – 169.032 -60.149 0.695 -7.063 0.383 28.35
Hunt & Reffert 2024 169.025 -60.141 0.695 -7.07 0.4 28.366
Cavallo et al. 2024 169.06 -60.155 0.695 – – –
Hunt & Reffert 2023 169.025 -60.141 0.695 -7.07 0.4 28.366

💡 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 – – – – – 114* – –
Cavallo et al. 2024 1.35 0.77 – 339 0.060 – – –
Hunt & Reffert 2023 1.37 0.61 0.40 208 – – – –

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

Visualization

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