FSR 0584

(SAI 20; MWSC 193)

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0.30 UTI
0.0
CN
0.18
Cdens
1.0
CC3
0.16
Clit
1.0
Cdup
Core radius and density 1.9 [pc], 0.9 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.18 Very loose
  • CC3 1.0 Very high quality
  • Clit 0.16 Rarely studied
  • Cdup 1.0 Unique

Overview

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FSR 0584 is a sparse, very loose object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 36.774 61.645 0.453 -0.718 -0.418 0.964
Just et al. 2023 36.789 61.626 – – – –
Kharchenko et al. 2016 36.789 61.626 – – – –
Kharchenko et al. 2013 36.802 61.628 – 1.19 0.55 –
Kharchenko et al. 2012 36.802 61.628 – 1.19 0.55 –
Glushkova et al. 2010 36.77 61.628 – – – –
Froebrich et al. 2007 36.796 61.628 – – – –
Dias et al. 2002 36.796 61.628 – 1.19 0.55 –

💡 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– 2.01 3.28 – 1259 – 202 – –
Just et al. 2023 – – – 1259 – 202 – –
Kharchenko et al. 2016 2.01 3.28 – 1259 – – – –
Kharchenko et al. 2013 2.01 3.28 – 1259 – – – –
Kharchenko et al. 2012 2.01 3.28 – 1259 – – – –
Dias et al. 2002 2.01 3.28 – 1259 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
IC1805-West 4.0 37.27 61.55 0.41 -0.96 -0.59 – 0.12

💡 Note: The % column shows the percentage of members that FSR 0584 shares with each listed object.

Visualization

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