HSC 243

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0.39 UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.71
Cdup
Radius (P>50% members) 4.4 [arcmin]
  • CN 0.77 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.71 Likely unique

Overview

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HSC 243 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 high extinction. It is catalogued as a massive, near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

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

Relatively close High extinction Massive Near-solar metallicity Very young

Cavallo et al. (2024)
Wood sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 279.081 -6.74 0.354 -0.139 -2.245 39.939
Hunt & Reffert 2024 279.073 -6.763 0.354 -0.136 -2.243 95.009
Cavallo et al. 2024 279.084 -6.726 0.355 – – –
Hunt & Reffert 2023 279.073 -6.763 0.354 -0.136 -2.243 95.009

💡 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 – – – – – 2594* – –
Cavallo et al. 2024 2.96 4.55 – 7 0.430 – – –
Hunt & Reffert 2023 2.59 4.50 3.04 12 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0045 28.8 279.08 -6.67 0.35 -0.15 -2.2 – 0.49
Ryu 865 3.4 279.19 -6.78 0.35 -0.27 -2.24 – 0.22

💡 Note: The % column shows the percentage of members that HSC 243 shares with each listed object.

Visualization

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