FSR 0823

(MWSC 650)

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0.31 UTI
0.0
CN
0.16
Cdens
0.5
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad) 0.8 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.16 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.45 Poorly studied
  • Cdup 1.0 Unique

Overview

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FSR 0823 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~2.81 kpc) differs significantly from the median photometric distance (~1.10 kpc).

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 85.654 29.559 0.355 1.083 -1.238 -14.703
Just et al. 2023 85.637 29.549 – – – –
Donor et al. 2020 85.645 29.548 – 1.3 -2.07 5.4
Bica et al. 2019 85.662 29.571 – – – –
Kharchenko et al. 2016 85.637 29.549 – – – –
Kharchenko et al. 2013 85.645 29.548 – 4.01 -2.45 –
Kharchenko et al. 2012 85.645 29.548 – 4.01 -2.45 –
Froebrich et al. 2007 85.658 29.566 – – – –
Dias et al. 2002 85.658 29.566 – 1.44 -4.71 –

💡 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– 1.1 1.71 – 638 -0.200 20 – –
Just et al. 2023 – – – 638 – 20 – –
Donor et al. 2020 – – – – -0.200 – – –
Kharchenko et al. 2016 1.10 1.71 – 638 – – – –
Kharchenko et al. 2013 1.10 1.71 – 638 – – – –
Kharchenko et al. 2012 1.10 1.71 – 638 – – – –
Dias et al. 2002 1.10 1.71 – 638 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2332 36.0 85.62 29.8 0.33 1.09 -1.27 -29.52 0.23

💡 Note: The % column shows the percentage of members that FSR 0823 shares with each listed object.

Visualization

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