Chupina 4

(MWSC 1590)

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0.35 UTI
0.0
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 7.5 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Chupina 4 is a sparse, very dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane. It is catalogued as a near-solar metallicity cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 6 years.

Note: This object shares a large percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 133.009 12.337 1.154 -10.931 -2.95 33.991
Donor et al. 2020 133.0 12.378 – -10.99 -2.86 33.8
Bica et al. 2019 132.998 12.377 – – – –
Dias et al. 2002 133.0 12.378 – 4.58 -14.11 –

💡 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] Bfrac BSS
UCC 99999– – – – – 0.000 – – –
Donor et al. 2020 – – – – 0.000 – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Melotte 94 100.0 132.85 11.82 1.15 -10.97 -2.91 33.91 1.0
CWWDL 14090 40.0 132.84 11.82 1.15 -10.98 -2.91 33.79 0.0

💡 Note: The % column shows the percentage of members that Chupina 4 shares with each listed object.

Visualization

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