FSR 1424

(MWSC 1582)

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0.68 UTI
0.79
CN
1.0
Cdens
0.75
CC3
0.44
Clit
1.0
Cdup
Radius (P>50% members) 8.2 [arcmin]
  • CN 0.79 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.44 Poorly studied
  • Cdup 1.0 Unique

Overview

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FSR 1424 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Relatively close High extinction 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 – 132.733 -43.837 0.426 -5.342 4.315 42.647
Hunt & Reffert 2024 132.691 -43.845 0.422 -5.307 4.308 37.267
Cavallo et al. 2024 132.706 -43.838 0.422 – – –
Hunt & Reffert 2023 132.691 -43.845 0.422 -5.307 4.308 37.267
Just et al. 2023 132.655 -43.829 – – – –
Kharchenko et al. 2016 132.655 -43.829 – – – –
Kharchenko et al. 2013 132.66 -43.832 – -13.1 6.29 –
Froebrich et al. 2007 132.667 -43.846 – – – –

💡 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
Hunt & Reffert 2024 – – – – – 321* – –
Cavallo et al. 2024 1.86 3.29 – 35 0.380 – – –
Hunt & Reffert 2023 2.27 3.48 1.89 17 – – – –
Just et al. 2023 – – – 251 – 21 – –
Kharchenko et al. 2016 1.83 3.74 – 251 – – – –
Kharchenko et al. 2013 1.83 3.74 – 251 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1444 82.3 132.73 -43.84 0.42 -5.4 4.31 37.24 0.04

💡 Note: The % column shows the percentage of members that FSR 1424 shares with each listed object.

Visualization

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