HSC 2599

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0.36 UTI
0.3
CN
1.0
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.1 [arcmin]
  • CN 0.3 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2599 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~6.05 kpc) differs significantly from the median photometric distance (~4.56 kpc).

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

Distant High extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 204.576 -63.423 0.165 -7.84 -1.664 -14.485
Hunt & Reffert 2024 204.576 -63.418 0.171 -7.839 -1.634 -14.486
Cavallo et al. 2024 204.57 -63.415 0.173 – – –
Hunt & Reffert 2023 204.576 -63.418 0.171 -7.839 -1.634 -14.486

💡 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 – – – – – 2234* – –
Cavallo et al. 2024 4.27 4.83 – 195 0.330 – – –
Hunt & Reffert 2023 4.85 5.05 2.71 157 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3998 100.0 204.58 -63.43 0.19 -7.8 -1.69 -26.39 0.34

💡 Note: The % column shows the percentage of members that HSC 2599 shares with each listed object.

Visualization

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