FoF 1199

(LP 1199)

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0.55 UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.9 [arcmin]
  • CN 0.77 Rich
  • 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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FoF 1199 is a rich, very dense object of very 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, near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.

Distant High extinction Massive Near-solar metallicity Young

Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 263.399 -34.445 0.277 -0.679 -1.528 -12.339
Almeida et al. 2025 263.389 -34.44 – – – –
Dias et al. 2021 263.389 -34.44 0.255 -0.584 -1.511 -12.02

💡 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
Almeida et al. 2025 3.30 3.69 – 24 – 1299 – –
Dias et al. 2021 3.30 3.69 – 24 0.378 – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0692 49.7 263.38 -34.45 0.28 -0.72 -1.56 -12.78 0.02

💡 Note: The % column shows the percentage of members that FoF 1199 shares with each listed object.

Visualization

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