FSR 1421

(MWSC 1608)

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0.26 UTI
0.0
CN
0.13
Cdens
0.25
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad) 0.6 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.13 Very loose
  • CC3 0.25 Low quality
  • Clit 0.45 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
FSR 1421 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is poorly studied in the literature.

Palma et al. (2025)
Classified as optical pair (not dynamically associated) P84, along with BH_56.

Cavallo et al. (2024)
Bronze sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 134.284 -42.506 0.963 -7.115 4.775 30.713
Hunt & Reffert 2024 134.451 -42.656 1.036 -6.716 3.982 13.201
Cavallo et al. 2024 134.56 -42.825 1.067 – – –
Hunt & Reffert 2023 134.451 -42.656 1.036 -6.716 3.982 13.201
Just et al. 2023 134.518 -42.597 – – – –
He et al. 2022 134.072 -42.428 0.955 -7.57 5.673 –
Kharchenko et al. 2016 134.518 -42.597 – – – –
Kharchenko et al. 2013 134.523 -42.6 – -8.76 9.08 –
Froebrich et al. 2007 134.537 -42.616 – – – –

💡 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– 1.155 2.26 2.75 125 -0.020 115 – –
Hunt & Reffert 2024 – – – – – 211(1) – –
Cavallo et al. 2024 1.04 2.17 – 6 -0.020 – – –
Hunt & Reffert 2023 0.90 2.26 2.75 7 – – – –
Just et al. 2023 – – – 200 – 19 – –
He et al. 2022 – 2.45 – 50 – – – –
Kharchenko et al. 2016 1.27 2.26 – 200 – – – –
Kharchenko et al. 2013 1.27 2.26 – 200 – – – –

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

Visualization

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