G3CC 58

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0.51 UTI
0.56
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 16.2 [N/pc2]
  • CN 0.56 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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G3CC 58 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. It is catalogued as a cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 13 years.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Morales et al. (2013)
Classified as morphological type 'OC1' (totally exposed cluster still physically associated with gas). Morphological flag: exposed cluster, without submm emission, presence of an IR bubble.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 279.083 -6.68 0.354 -0.14 -2.232 17.899
Morales et al. 2013 279.085 -6.649 – – – –

💡 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– 2.92 – – – – – – –
Morales et al. 2013 2.92 – – – – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 243 98.4 279.08 -6.74 0.35 -0.14 -2.24 39.94 0.32
OC 0045 65.1 279.08 -6.67 0.35 -0.15 -2.2 – 0.02

💡 Note: The % column shows the percentage of members that G3CC 58 shares with each listed object.

Visualization

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