HSC 1329

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0.39 UTI
0.76
CN
0.33
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 6.4 [arcmin]
  • CN 0.76 Rich
  • Cdens 0.33 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1329 is a rich, loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
Distant Moderate extinction Massive Near-solar metallicity Young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 82.471 38.477 0.222 0.358 -0.518 –
Zhang et al. 2024 82.462 38.462 – – – –
Hunt & Reffert 2024 82.462 38.462 0.237 0.355 -0.51 -7.916
Cavallo et al. 2024 82.49 38.459 0.231 – – –
Hunt & Reffert 2023 82.462 38.462 0.237 0.355 -0.51 -7.916

💡 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
Zhang et al. 2024 – – – – -0.104* – – –
Hunt & Reffert 2024 – – – – – 1101* – –
Cavallo et al. 2024 4.83 2.56 – 98 0.690 – – –
Hunt & Reffert 2023 3.84 2.89 2.72 31 – – – –

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

Visualization

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