HSC 412

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0.35 UTI
0.31
CN
0.71
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 0.71 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 412 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
Distant Very high extinction Massive Near-solar metallicity Very 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 – 290.598 15.136 0.227 -2.176 -5.341 13.462
Hunt & Reffert 2024 290.596 15.14 0.231 -2.173 -5.335 –
Cavallo et al. 2024 290.594 15.149 0.237 – – –
Hunt & Reffert 2023 290.596 15.14 0.231 -2.173 -5.335 –

💡 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 – – – – – 1657* – –
Cavallo et al. 2024 5.78 5.21 – 7 0.000 – – –
Hunt & Reffert 2023 3.96 6.23 2.19 11 – – – –

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

Visualization

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