FSR 0213

(MWSC 3342)

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0.20 UTI
0.0
CN
0.02
Cdens
0.12
CC3
0.44
Clit
1.0
Cdup
Radius (P>50% members) 31.0 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.02 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.44 Poorly studied
  • Cdup 1.0 Unique

Overview

FSR 0213 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Relatively close Moderate extinction Intermediate age

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 306.631 38.936 0.879 -0.485 -3.186 15.969
Just et al. 2023 306.74 38.97
He et al. 2022 306.13 39.026 1.024 -1.503 -3.574
Bica et al. 2019 306.748 38.977
Kharchenko et al. 2016 306.74 38.97
Kharchenko et al. 2013 306.745 38.972 -2.59 -3.73
Froebrich et al. 2007 306.746 38.976
Dias et al. 2002 306.746 38.976 -0.53 -3.16

💡 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 519 69
He et al. 2022 3.35 5
Kharchenko et al. 2016 1.43 2.58 519
Kharchenko et al. 2013 1.43 2.58 519
Dias et al. 2002 1.43 2.58 519

💡 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.