HSC 2539

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0.51 UTI
0.78
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.0 [arcmin]
  • CN 0.78 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2539 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a very massive, near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Distant High extinction Very massive Near-solar metallicity 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 – 193.86 -63.03 0.237 -6.259 -0.433 -43.908
Hunt & Reffert 2024 193.855 -63.04 0.234 -6.268 -0.433 -6.92
Cavallo et al. 2024 193.866 -63.028 0.24 – – –
Hunt & Reffert 2023 193.855 -63.04 0.234 -6.268 -0.433 -6.92

💡 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 – – – – – 5026* – –
Cavallo et al. 2024 3.28 5.01 – 74 -0.070 – – –
Hunt & Reffert 2023 3.76 4.96 3.08 39 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3244 99.0 193.86 -63.03 0.24 -6.26 -0.44 -43.75 0.12

💡 Note: The % column shows the percentage of members that HSC 2539 shares with each listed object.

Visualization

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