FSR 1452

(MWSC 1597; FoF 107)

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0.82 UTI
0.83
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members) 5.3 [arcmin]
  • CN 0.83 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.75 Well-studied
  • Cdup 1.0 Unique

Overview

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FSR 1452 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is well-studied in the literature.
Relatively close Moderate extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 133.319 -47.867 0.384 -4.596 3.789 20.4
Li et al. 2025 133.332 -47.871 0.363 -4.603 3.722 –
Hunt & Reffert 2024 133.328 -47.855 0.387 -4.601 3.833 20.307
Cavallo et al. 2024 133.27 -47.828 0.386 – – –
Hunt & Reffert 2023 133.328 -47.855 0.387 -4.601 3.833 20.307
Just et al. 2023 133.322 -47.917 – – – –
Cantat-Gaudin et al. 2020 133.332 -47.871 0.363 -4.603 3.722 –
Cantat-Gaudin & Anders 2020 133.332 -47.871 0.363 -4.603 3.722 –
Liu & Pang 2019 133.319 -47.862 0.377 -4.566 3.812 –
Soubiran et al. 2018 133.332 -47.871 – – – 16.23
Cantat-Gaudin et al. 2018 133.332 -47.871 0.363 -4.603 3.722 –
Kharchenko et al. 2016 133.322 -47.917 – – – –
Kharchenko et al. 2013 133.327 -47.92 – -2.74 10.15 –
Froebrich et al. 2007 133.283 -47.92 – – – –

💡 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] Bfr BSS
Li et al. 2025 2.22 2.01 – 224 -0.043 – – –
Hunt & Reffert 2024 – – – – – 1920* – –
Cavallo et al. 2024 2.49 2.33 – 148 0.310 – – –
Hunt & Reffert 2023 2.33 1.98 2.62 164 – – – –
Just et al. 2023 – – – 1122 – 129 – –
Cantat-Gaudin et al. 2020 2.30 1.49 – 234 – – – –
Cantat-Gaudin & Anders 2020 2.55 – – – – – – –
Liu & Pang 2019 – – – 977 -2.000 – – –
Soubiran et al. 2018 2.55 – – – – – – –
Cantat-Gaudin et al. 2018 2.55 – – – – – – –
Kharchenko et al. 2016 2.07 1.16 – 1122 – – – –
Kharchenko et al. 2013 2.07 1.16 – 1122 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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