FSR 0330

(MWSC 3639)

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0.25 UTI
0.0
CN
0.11
Cdens
0.38
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members) 5.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.11 Very loose
  • CC3 0.38 Low quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

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FSR 0330 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 moderate extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.79 kpc) differs significantly from the median photometric distance (~1.90 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.

Relatively close Moderate 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 – 338.523 43.335 0.264 -2.388 -3.166 14.254
Just et al. 2023 338.541 43.337 – – – –
Bica et al. 2019 338.542 43.347 – – – –
Kharchenko et al. 2016 338.541 43.337 – – – –
Kharchenko et al. 2013 338.548 43.34 – -1.86 -1.45 –
Kharchenko et al. 2012 338.548 43.34 – -1.86 -1.45 –
Froebrich et al. 2007 338.533 43.348 – – – –

💡 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 – – – 1365 – 221 – –
Kharchenko et al. 2016 1.90 1.24 – 1365 – – – –
Kharchenko et al. 2013 1.90 1.24 – 1365 – – – –
Kharchenko et al. 2012 1.90 1.24 – 1365 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 0331 36.0 338.63 43.44 0.24 -2.46 -3.06 -48.97 0.22

💡 Note: The % column shows the percentage of members that FSR 0330 shares with each listed object.

Visualization

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