FSR 1082

(MWSC 951)

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0.08 UTI
0.0
CN
0.01
Cdens
0.25
CC3
0.06
Clit
1.0
Cdup
Core radius and density 8.6 [pc], 0.06 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.01 Very loose
  • CC3 0.25 Low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

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FSR 1082 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

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– 100.038 -1.737 0.218 -0.48 0.101 59.383
Just et al. 2023 100.02 -1.743 – – – –
Kharchenko et al. 2016 100.02 -1.743 – – – –
Kharchenko et al. 2013 100.027 -1.745 – 2.42 1.83 –
Froebrich et al. 2007 100.042 -1.72 – – – –

💡 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– 4.04 2.63 – 692 – 2198 – –
Just et al. 2023 – – – 692 – 2198 – –
Kharchenko et al. 2016 4.04 2.63 – 692 – – – –
Kharchenko et al. 2013 4.04 2.63 – 692 – – – –

Visualization

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