SAI 48

(MWSC 529; Teutsch 37)

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0.11 UTI
0.0
CN
0.11
Cdens
0.38
CC3
0.45
Clit
0.4
Cdup
Stellar density (N50/rad) 0.5 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.11 Very loose
  • CC3 0.38 Low quality
  • Clit 0.45 Poorly studied
  • Cdup 0.4 Possibly duplicate

Overview

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SAI 48 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 an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously 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– 80.864 33.487 0.299 -0.148 -1.257 40.832
Just et al. 2023 81.046 33.477 – – – –
Bica et al. 2019 81.071 33.506 – – – –
Kharchenko et al. 2016 81.046 33.477 – – – –
Dias et al. 2014 81.071 33.501 – 0.75 -2.45 –
Kharchenko et al. 2013 81.055 33.477 – 5.08 -5.66 –
Kharchenko et al. 2012 81.055 33.477 – 5.08 -5.66 –
Glushkova et al. 2010 81.07 33.501 – – – –
Dias et al. 2002 81.071 33.501 – 0.75 -2.45 –

💡 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– 4.0 2.48 – 891 – 638 – –
Just et al. 2023 – – – 891 – 638 – –
Kharchenko et al. 2016 4.00 2.48 – 891 – – – –
Kharchenko et al. 2013 4.00 2.48 – 891 – – – –
Kharchenko et al. 2012 4.00 2.48 – 891 – – – –
Glushkova et al. 2010 1.80 0.96 – 2239 – – – –
Dias et al. 2002 1.80 0.96 – 2239 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
NGC 1893 60.0 80.73 33.45 0.3 -0.28 -1.41 20.89 0.92

💡 Note: The % column shows the percentage of members that SAI 48 shares with each listed object.

Visualization

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