FSR 1447

(MWSC 1445)

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0.18 UTI
0.0
CN
0.16
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 6.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.16 Very loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

FSR 1447 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 old cluster (see Parameters). It is poorly studied in the literature.

⚠️ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Moderate extinction Old

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 122.91 -51.014 0.36 -3.718 6.439
Just et al. 2023 122.884 -51.018
Kharchenko et al. 2016 122.884 -51.018
Kharchenko et al. 2013 122.887 -51.02 -3.0 2.85
Froebrich et al. 2007 122.883 -51.024

💡 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
Just et al. 2023 1259 62
Kharchenko et al. 2016 2.55 2.58 1259
Kharchenko et al. 2013 2.55 2.58 1259

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.

Visualization

Galactocentric position diagram

💡 Note: How are the galactocentric plots generated? See FAQ.