FSR 1350

(MWSC 1341)

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0.31 UTI
0.32
CN
0.23
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.2 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 0.23 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
FSR 1350 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.51 kpc) differs significantly from the median photometric distance (~1.61 kpc).

Note: This object shares a very small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

âš ī¸ 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 Intermediate age

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 116.932 -34.041 0.285 -2.068 3.063 –
Just et al. 2023 116.945 -34.034 – – – –
Kharchenko et al. 2016 116.945 -34.034 – – – –
Kharchenko et al. 2013 116.95 -34.036 – -5.43 5.89 –
Froebrich et al. 2007 116.95 -34.036 – – – –

💡 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 – – – 398 – 109 – –
Kharchenko et al. 2016 1.61 2.58 – 398 – – – –
Kharchenko et al. 2013 1.61 2.58 – 398 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 1347 3.1 117.03 -33.71 0.26 -2.15 3.12 110.58 0.76

💡 Note: The % column shows the percentage of members that FSR 1350 shares with each listed object.

Visualization

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