FSR 0519

(MWSC 83; FoF 550)

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0.77 UTI
0.59
CN
0.77
Cdens
1.0
CC3
0.75
Clit
1.0
Cdup
C3 classification AA
Number of members (P>50%) 68
Radius (P>50% members) 4.9 [arcmin]
  • CN 0.59 Moderately populated
  • Cdens 0.77 Dense
  • CC3 1.0 Very high quality
  • Clit 0.75 Well-studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
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FSR 0519 is a moderately populated, dense object of very high C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is well-studied in the literature.

(*): The parallax distance estimate (~2.94 kpc) differs significantly from the median photometric distance (~2.09 kpc).

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data
🔍 Search references for FSR 0519 in: SciX Simbad
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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 13.155 64.628 0.34 -2.433 -0.379 –
Hunt & Reffert 2024 13.161 64.617 0.343 -2.439 -0.377 -66.704
Cavallo et al. 2024 12.987 64.582 0.344 – – –
Hunt & Reffert 2023 13.161 64.617 0.343 -2.439 -0.377 -66.704
Just et al. 2023 13.112 64.663 – – – –
Cantat-Gaudin & Anders 2020 13.092 64.596 0.324 -2.423 -0.331 –
Liu & Pang 2019 13.179 64.618 0.35 -2.437 -0.276 –
Cantat-Gaudin et al. 2019 13.092 64.596 0.32 -2.42 -0.33 –
Bica et al. 2019 13.135 64.651 – – – –
Kharchenko et al. 2016 13.112 64.663 – – – –
Kharchenko et al. 2013 13.122 64.667 – 0.03 2.47 –
Kharchenko et al. 2012 13.122 64.667 – -0.68 1.43 –
Froebrich et al. 2007 13.125 64.651 – – – –
Dias et al. 2002 13.125 64.651 – -5.38 -2.55 –

💡 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] Bfr BSS
Hunt & Reffert 2024 – – – – – 947* – –
Cavallo et al. 2024 2.86 2.38 – 60 0.190 – – –
Hunt & Reffert 2023 2.66 2.36 1.92 53 – – – –
Just et al. 2023 – – – 22 – 69 – –
Cantat-Gaudin & Anders 2020 2.83 – – – – – – –
Liu & Pang 2019 – – – 6 0.500 – – –
Cantat-Gaudin et al. 2019 2.83 – – – – – – –
Kharchenko et al. 2016 1.52 2.16 – 22 – – – –
Kharchenko et al. 2013 1.52 2.16 – 22 – – – –
Kharchenko et al. 2012 1.45 2.17 – 1660 – – – –
Dias et al. 2002 1.45 2.17 – 1660 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1209 98.5 13.11 64.61 0.35 -2.44 -0.38 -66.72 0.23
UBC 411 61.8 13.11 64.62 0.34 -2.43 -0.36 – 0.06

💡 Note: The % column shows the percentage of members that FSR 0519 shares with each listed object.

Visualization
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FSR 0519 UCC
FSR 0519 HUNT23
Galactocentric position diagram