FSR 0331

(MWSC 3640)

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0.22 UTI
0.0
CN
0.12
Cdens
0.25
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members) 4.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.12 Very loose
  • CC3 0.25 Low quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
FSR 0331 is a sparse, 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 (~4.23 kpc) differs significantly from the median photometric distance (~3.00 kpc).

Note: This object shares a moderate 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.

Distant Low extinction Old

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 338.633 43.443 0.236 -2.456 -3.065 -48.97
Just et al. 2023 338.678 43.437 – – – –
Bica et al. 2019 338.647 43.428 – – – –
Kharchenko et al. 2016 338.678 43.437 – – – –
Kharchenko et al. 2013 338.685 43.44 – -3.19 -1.09 –
Kharchenko et al. 2012 338.685 43.44 – -3.19 -1.09 –
Froebrich et al. 2007 338.65 43.429 – – – –

💡 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 – – – 1995 – 628 – –
Kharchenko et al. 2016 3.00 0.13 – 1995 – – – –
Kharchenko et al. 2013 3.00 0.13 – 1995 – – – –
Kharchenko et al. 2012 3.00 0.13 – 1995 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 0330 36.0 338.52 43.34 0.26 -2.39 -3.17 14.25 0.25

💡 Note: The % column shows the percentage of members that FSR 0331 shares with each listed object.

Visualization

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