HSC 92

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0.03 UTI
0.81
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.04
Cdup
Radius (P>50% members) 2.6 [arcmin]
  • CN 0.81 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.04 Very likely duplicate

Overview

â„šī¸
HSC 92 is a rich, very dense object of very 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 very massive, metal-poor, 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.

Relatively close Very high extinction Very massive Metal-poor 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 – 269.494 -23.289 0.285 -0.069 -1.674 -11.29
Hunt & Reffert 2024 269.497 -23.292 0.283 -0.098 -1.68 -9.233
Cavallo et al. 2024 269.498 -23.277 0.282 – – –
Hunt & Reffert 2023 269.497 -23.292 0.283 -0.098 -1.68 -9.233

💡 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 – – – – – 7637* – –
Cavallo et al. 2024 2.43 5.48 – 105 -0.550 – – –
Hunt & Reffert 2023 3.08 5.15 3.20 41 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 1625 95.5 269.5 -23.29 0.3 -0.09 -1.64 -11.45 0.57

💡 Note: The % column shows the percentage of members that HSC 92 shares with each listed object.

Visualization

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