SAI 90

(MWSC 1493)

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0.30 UTI
0.0
CN
0.16
Cdens
0.25
CC3
0.55
Clit
1.0
Cdup
Stellar density (N50/rad) 0.8 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.16 Very loose
  • CC3 0.25 Low quality
  • Clit 0.55 Moderately studied
  • Cdup 1.0 Unique

Overview

â„šī¸
SAI 90 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a very metal-rich, old cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is moderately studied in the literature.

Palma et al. (2025)
Classified as tidal capture (resonant trapping pair) P7, along with CWNU_1656.

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 127.018 -41.751 0.414 -4.849 4.335 –
Hunt & Reffert 2024 127.026 -41.754 0.418 -4.822 4.335 14.297
Cavallo et al. 2024 126.702 -41.79 0.418 – – –
Hunt & Reffert 2023 127.026 -41.754 0.418 -4.822 4.335 14.297
Just et al. 2023 127.018 -41.767 – – – –
Bica et al. 2019 126.997 -41.767 – – – –
Kharchenko et al. 2016 127.018 -41.767 – – – –
Dias et al. 2014 126.996 -41.769 – -1.91 1.81 –
Kharchenko et al. 2013 127.023 -41.77 – -3.79 6.32 –
Glushkova et al. 2010 126.995 -41.769 – – – –
Dias et al. 2002 126.996 -41.769 – -1.91 1.81 –

💡 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– 2.74 3.16 2.69 1122 1.040 328 – –
Hunt & Reffert 2024 – – – – – 248(1) – –
Cavallo et al. 2024 2.56 2.99 – 38 1.040 – – –
Hunt & Reffert 2023 2.21 2.72 2.69 13 – – – –
Just et al. 2023 – – – 1274 – 409 – –
Kharchenko et al. 2016 3.11 3.23 – 1274 – – – –
Kharchenko et al. 2013 3.11 3.23 – 1274 – – – –
Glushkova et al. 2010 2.74 3.16 – 1122 – – – –
Dias et al. 2002 2.74 3.16 – 1122 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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