FSR 0112

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0.07 UTI
0.0
CN
0.11
Cdens
0.12
CC3
0.06
Clit
1.0
Cdup
Stellar density (N50/rad) 0.6 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.11 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
FSR 0112 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, well below the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~2.78 kpc) differs significantly from the median photometric distance (~1.22 kpc).

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 302.119 -3.539 0.36 -3.222 -6.574 25.591
Bica et al. 2019 302.081 -3.541 – – – –
Dib et al. 2018 302.107 -3.543 – – – –
Joshi et al. 2016 302.107 -3.543 – – – –
Froebrich et al. 2007 302.083 -3.538 – – – –

💡 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– 1.22 0.66 – 2213 – – – –
Dib et al. 2018 1.22 – – 2213 – – – –
Joshi et al. 2016 1.22 0.66 – 2213 – – – –

Visualization

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