HSC 1172

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0.00 UTI
0.6
CN
0.6
Cdens
0.75
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members) 3.5 [arcmin]
  • CN 0.6 Moderately populated
  • Cdens 0.6 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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HSC 1172 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, above 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.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large 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 – 61.544 58.413 0.21 -0.19 0.005 -82.763
Hunt & Reffert 2024 61.557 58.441 0.22 -0.179 0.016 -82.757
Cavallo et al. 2024 61.57 58.404 0.214 – – –
Hunt & Reffert 2023 61.557 58.441 0.22 -0.179 0.016 -82.757

💡 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 – – – – – 809* – –
Cavallo et al. 2024 4.59 2.09 – 110 0.610 – – –
Hunt & Reffert 2023 4.04 2.31 1.72 38 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 613 100.0 61.54 58.41 0.22 -0.17 0.0 -67.35 0.48

💡 Note: The % column shows the percentage of members that HSC 1172 shares with each listed object.

Visualization

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