FSR 0481

(MWSC 48)

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0.20 UTI
0.0
CN
0.02
Cdens
0.38
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 8.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.02 Very loose
  • CC3 0.38 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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FSR 0481 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large* 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 (~5.72 kpc) differs significantly from the median photometric distance (~2.16 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 – 7.235 43.288 0.175 -1.834 -1.471 -50.169
Just et al. 2023 7.226 43.276 – – – –
Kharchenko et al. 2016 7.226 43.276 – – – –
Kharchenko et al. 2013 7.234 43.279 – 3.5 1.31 –
Kharchenko et al. 2012 7.234 43.279 – 3.5 1.31 –
Froebrich et al. 2007 7.237 43.29 – – – –

💡 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 – – – 1259 – 140 – –
Kharchenko et al. 2016 2.16 1.19 – 1259 – – – –
Kharchenko et al. 2013 2.16 1.19 – 1259 – – – –
Kharchenko et al. 2012 2.37 1.19 – 1259 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 0483 28.0 7.29 43.25 0.37 -2.72 -2.42 -67.42 0.37

💡 Note: The % column shows the percentage of members that FSR 0481 shares with each listed object.

Visualization

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