HSC 796

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0.05 UTI
0.54
CN
0.44
Cdens
0.38
CC3
0.0
Clit
0.17
Cdup
Radius (P>50% members) 2.8 [arcmin]
  • CN 0.54 Moderately populated
  • Cdens 0.44 Loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.17 Likely duplicate

Overview

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HSC 796 is a moderately populated, loose object of low C3 quality. Its parallax locates it at a large distance, above 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.

âš ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Very distant High 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 – 332.632 57.737 0.158 -2.861 -2.018 -58.941
Hunt & Reffert 2024 332.592 57.765 0.164 -2.868 -2.039 -48.449
Cavallo et al. 2024 332.656 57.732 0.161 – – –
Hunt & Reffert 2023 332.592 57.765 0.164 -2.868 -2.039 -48.449

💡 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 – – – – – 1726* – –
Cavallo et al. 2024 6.67 3.88 – 36 0.280 – – –
Hunt & Reffert 2023 6.16 3.79 2.63 42 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3072 89.7 332.61 57.74 0.16 -2.86 -2.02 – 0.03
FSR 0354 82.8 332.75 57.69 0.17 -2.89 -2.03 -48.45 0.45
LP 24 6.9 332.61 57.86 0.2 -2.85 -1.79 – 0.14

💡 Note: The % column shows the percentage of members that HSC 796 shares with each listed object.

Visualization

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