GGD 12-15

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0.50 UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 97.1 [N/pc2]
  • CN 0.75 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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GGD 12-15 is a rich, very dense object of high C3 quality. Its parallax locates it at a close distance, below 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 23 years.

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

Lada & Lada (2003)
Embedded cluster within âˆŧ2 Kpc of the Sun.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 92.691 -6.212 1.208 -3.579 0.48 35.635
Lada & Lada 2003 92.712 -6.198 – – – –

💡 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– 0.8 – – – – 73 – –
Lada & Lada 2003 0.80 – – – – 73 – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
NGC 2183 55.0 92.69 -6.24 1.19 -3.63 0.4 25.06 0.44
OC 0358 3.7 93.11 -6.38 1.17 -3.88 0.35 27.82 0.19

💡 Note: The % column shows the percentage of members that GGD 12-15 shares with each listed object.

Visualization

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