HSC 797

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0.30 UTI
0.48
CN
0.64
Cdens
0.75
CC3
0.0
Clit
0.79
Cdup
Radius (P>50% members) 3.2 [arcmin]
  • CN 0.48 Poorly populated
  • Cdens 0.64 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.79 Very likely unique

Overview

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HSC 797 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 moderate extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

Distant Moderate extinction Metal-rich 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 – 334.836 55.988 0.241 -3.566 -2.637 –
Hunt & Reffert 2024 334.831 55.983 0.238 -3.545 -2.655 –
Cavallo et al. 2024 334.92 55.978 0.238 – – –
Hunt & Reffert 2023 334.831 55.983 0.238 -3.545 -2.655 –

💡 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 – – – – – 745* – –
Cavallo et al. 2024 3.87 2.00 – 79 0.720 – – –
Hunt & Reffert 2023 4.07 2.11 1.21 13 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Teutsch 127 20.8 334.75 56.1 0.24 -3.37 -2.51 -60.77 0.78

💡 Note: The % column shows the percentage of members that HSC 797 shares with each listed object.

Visualization

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