FSR 1227

(MWSC 1256)

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0.25 UTI
0.0
CN
0.13
Cdens
0.38
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members) 5.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.13 Very loose
  • CC3 0.38 Low quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

FSR 1227 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Distant Moderate extinction Intermediate age

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 112.95 -13.843 0.305 -2.474 2.624 52.336
Just et al. 2023 112.973 -13.833
Bica et al. 2019 112.967 -13.861
Kharchenko et al. 2016 112.973 -13.833
Kharchenko et al. 2013 112.98 -13.835 -1.51 4.26
Froebrich et al. 2007 112.971 -13.86
Dias et al. 2002 112.971 -13.86 -1.51 4.26

💡 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 944 685
Kharchenko et al. 2016 4.50 1.29 944
Kharchenko et al. 2013 4.50 1.29 944
Dias et al. 2002 4.50 1.29 944

💡 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.