Saurer 6

(MWSC 3193; FSR 0180)

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0.33 UTI
0.0
CN
0.01
Cdens
0.62
CC3
0.5
Clit
1.0
Cdup
Stellar density (N50/rad) 0.0 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.01 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.5 Moderately studied
  • Cdup 1.0 Unique

Overview

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Saurer 6 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, old cluster (see Parameters). It is moderately studied in the literature.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 297.768 32.23 0.124 -2.759 -4.505 -57.162
He et al. 2023 297.755 32.244 0.073 -2.548 -4.057 -80.41
Just et al. 2023 297.753 32.231 – – – –
Perren et al. 2022 297.75 32.25 – – – –
Bica et al. 2019 297.769 32.238 – – – –
Kharchenko et al. 2016 297.753 32.231 – – – –
Dias et al. 2014 297.758 32.243 – -1.84 -1.38 –
Kharchenko et al. 2013 297.759 32.233 – -3.95 -0.61 –
van den Bergh 2006 297.75 32.25 – – – –
Dias et al. 2002 297.758 32.243 – -2.08 -1.56 –

💡 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– 8.955 2.65 – 1585 -0.110 3664 0.52 –
He et al. 2023 8.71 2.90 – 1259 – – – –
Just et al. 2023 – – – 1585 – 2128 – –
Perren et al. 2022 9.20 2.91 – 1380 -0.110 5200 0.52 –
Kharchenko et al. 2016 7.33 2.65 – 1585 – – – –
Kharchenko et al. 2013 7.33 2.65 – 1585 – – – –
van den Bergh 2006 9.33 2.39 – 1950 – – – –
Dias et al. 2002 9.33 2.39 – 1950 – – – –

Visualization

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