HSC 2642

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0.49 UTI
0.69
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.2 [arcmin]
  • CN 0.69 Moderately populated
  • 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 2642 is a moderately populated, 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 massive, metal-rich, very 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 Massive Metal-rich 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 – 213.787 -61.863 0.261 -3.982 -2.202 13.048
Hunt & Reffert 2024 213.797 -61.858 0.266 -3.987 -2.209 60.657
Cavallo et al. 2024 213.715 -61.897 0.256 – – –
Hunt & Reffert 2023 213.797 -61.858 0.266 -3.987 -2.209 60.657

💡 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 – – – – – 1188* – –
Cavallo et al. 2024 3.10 4.80 – 13 0.690 – – –
Hunt & Reffert 2023 3.33 4.33 3.17 19 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3944 77.3 213.79 -61.86 0.27 -3.97 -2.2 13.05 0.03

💡 Note: The % column shows the percentage of members that HSC 2642 shares with each listed object.

Visualization

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