FSR 0213

(MWSC 3342)

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0.16 UTI
0.0
CN
0.01
Cdens
0.12
CC3
0.32
Clit
1.0
Cdup
Core radius and density 5.1 [pc], 0.06 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.01 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.32 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
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, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

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.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 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 – – – –
Dias et al. 2018 – – – 0.81 -2.08 –
Dib et al. 2018 306.745 38.972 – – – –
Sampedro et al. 2017 306.746 38.976 – -0.86 -4.21 –
Joshi et al. 2016 306.745 38.972 – – – –
Kharchenko et al. 2016 306.74 38.97 – – – –
Dias et al. 2014 306.746 38.976 – -0.58 -3.23 –
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] Bfrac BSS
UCC 99999– 1.43 2.63 – 519 – 69 – –
Just et al. 2023 – – – 519 – 69 – –
He et al. 2022 – 3.35 – 5 – – – –
Dib et al. 2018 1.43 – – 519 – – – –
Joshi et al. 2016 1.43 2.63 – 519 – – – –
Kharchenko et al. 2016 1.43 2.63 – 519 – – – –
Kharchenko et al. 2013 1.43 2.63 – 519 – – – –
Dias et al. 2002 1.43 2.63 – 519 – – – –

Visualization

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