FSR 1607

(MWSC 1955)

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0.27 UTI
0.25
CN
0.23
Cdens
0.25
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 7.0 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.23 Very loose
  • CC3 0.25 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

FSR 1607 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, well below the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~2.31 kpc) differs significantly from the median photometric distance (~1.56 kpc).

Relatively close Low extinction Old

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 173.269 -77.882 0.433 -8.756 1.617 -51.456
Just et al. 2023 173.243 -77.822
Bica et al. 2019 173.231 -77.813
Kharchenko et al. 2016 173.243 -77.822
Kharchenko et al. 2013 173.25 -77.825 -8.99 -1.53
Froebrich et al. 2007 173.242 -77.817

💡 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 3673 164
Kharchenko et al. 2016 1.56 0.32 3673
Kharchenko et al. 2013 1.56 0.32 3673

💡 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.