Cmg 119

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0.48 UTI
0.29
CN
1.0
Cdens
1.0
CC3
0.06
Clit
1.0
Cdup
Core radius and density 0.7 [pc], 8.9 [pc-2]
  • CN 0.29 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Cmg 119 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is rarely studied in the literature.

Cavallo et al. (2024)
Wood sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.71 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.71 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 88.416 -10.409 1.343 -1.313 1.799 25.115
Hunt & Reffert 2024 88.415 -10.394 1.325 -1.254 1.877 27.696
Cavallo et al. 2024 88.383 -10.436 1.32 – – –
Hunt & Reffert 2023 88.415 -10.394 1.325 -1.254 1.877 27.696
Bica et al. 2019 88.424 -10.402 – – – –

💡 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– 0.73 3.2 1.89 6 -0.270 91 – –
Hunt & Reffert 2024 0.73 3.20 1.89 6 – 91(1) – –
Cavallo et al. 2024 2.00 2.12 – 18 -0.270 – – –
Hunt & Reffert 2023 0.73 3.20 1.89 6 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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