FSR 0505

(SAI 8)

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0.72 UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.55
Clit
1.0
Cdup
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.55 Moderately studied
  • Cdup 1.0 Unique

Overview

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FSR 0505 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, old cluster (see Parameters). It is moderately studied in the literature.

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

Very distant Moderate extinction Massive Near-solar metallicity Old

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 10.046 61.567 0.141 -0.931 -0.487 -64.074
Hu & Soubiran 2025 10.054 61.559 – – – –
Hunt & Reffert 2024 10.06 61.574 0.145 -0.935 -0.47 -69.696
Cavallo et al. 2024 10.054 61.559 0.135 – – –
Hunt & Reffert 2023 10.06 61.574 0.145 -0.935 -0.47 -69.696
Bica et al. 2019 10.017 61.602 – – – –
Dias et al. 2014 10.017 61.598 – -1.8 -0.25 –
Glushkova et al. 2010 10.037 61.568 – – – –
Froebrich et al. 2007 10.017 61.598 – – – –
Dias et al. 2002 10.017 61.598 – -2.03 -0.19 –

💡 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
Hu & Soubiran 2025 – – – – -0.290* – – –
Hunt & Reffert 2024 – – – – – 1024* – –
Cavallo et al. 2024 4.41 2.07 – 1175 -0.350 – – –
Hunt & Reffert 2023 6.05 2.40 1.68 455 – – – –
Glushkova et al. 2010 7.20 0.93 – 1413 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3330 82.2 10.05 61.56 0.14 -0.94 -0.5 -64.07 0.0

💡 Note: The % column shows the percentage of members that FSR 0505 shares with each listed object.

Visualization

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