HSC 2639

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0.44 UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.8
Cdup
Radius (P>50% members) 3.5 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.8 Very likely unique

Overview

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HSC 2639 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, metal-rich, very young cluster (see Parameters). It was recently reported in the literature.

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

Distant High extinction Massive Metal-rich Very young

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 – 213.026 -62.036 0.241 -6.05 -2.369 -39.078
Hunt & Reffert 2024 213.062 -62.041 0.241 -6.042 -2.357 -47.287
Cavallo et al. 2024 212.892 -62.047 0.242 – – –
Hunt & Reffert 2023 213.062 -62.041 0.241 -6.042 -2.357 -47.287

💡 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 – – – – – 4867* – –
Cavallo et al. 2024 3.84 4.40 – 14 0.770 – – –
Hunt & Reffert 2023 3.73 4.63 2.89 15 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0607 19.5 213.03 -62.02 0.2 -6.05 -2.37 – 0.26

💡 Note: The % column shows the percentage of members that HSC 2639 shares with each listed object.

Visualization

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