FSR 1243

(MWSC 1269)

Click to load Aladin Lite
0.18 UTI
0.0
CN
0.04
Cdens
0.12
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members) 7.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.04 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

FSR 1243 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is poorly studied in the literature.
Distant Moderate extinction Very young

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 113.611 -15.968 0.241 -2.293 2.537 117.33
Just et al. 2023 113.623 -15.933
Bica et al. 2019 113.637 -15.969
Kharchenko et al. 2016 113.623 -15.933
Kharchenko et al. 2013 113.629 -15.935 -1.02 0.03
Froebrich et al. 2007 113.638 -15.973
Dias et al. 2002 113.638 -15.973 -1.02 0.03

💡 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 5 479
Kharchenko et al. 2016 4.34 2.06 5
Kharchenko et al. 2013 4.34 2.06 5
Dias et al. 2002 4.34 2.06 5

💡 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.