FSR 0716

(SAI 44; MWSC 482)

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0.92 UTI
0.85
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
C3 classification AB
Number of members (P>50%) 368
Radius (P>50% members) 5.3 [arcmin]
  • CN 0.85 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique
πŸ“₯ Members πŸ“Š Colab πŸ”¬ Bayestar19 πŸ” CDS πŸ” Simbad πŸ” CDS (Ξ±, Ξ΄) πŸ” Simbad (Ξ±, Ξ΄)

Overview
ℹ️
FSR 0716 is a rich, very dense object of 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, intermediate-age cluster (see Parameters). It is very well-studied in the literature.
Distant Moderate extinction Near-solar metallicity Intermediate age

Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.

Cavallo et al. (2024)
Gold sample.

Data
πŸ” Search references for FSR 0716 in: SciX Simbad
ℹ️
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 77.788 45.722 0.259 -0.265 -1.666 -8.656
Li et al. 2025 77.786 45.718 0.252 -0.265 -1.628 –
Hu & Soubiran 2025 77.781 45.72 – – – –
Almeida et al. 2025 77.782 45.712 – – – –
Zhang et al. 2024 77.793 45.723 – – – –
Hunt & Reffert 2024 77.793 45.723 0.252 -0.323 -1.701 10.976
Cavallo et al. 2024 77.781 45.72 0.251 – – –
Hunt & Reffert 2023 77.793 45.723 0.252 -0.323 -1.701 10.976
Almeida et al. 2023 77.791 45.712 – – – –
Dias et al. 2021 77.782 45.712 0.249 -0.286 -1.636 –
Cantat-Gaudin et al. 2020 77.786 45.718 0.252 -0.265 -1.628 –
SΓ‘nchez et al. 2020 77.792 45.713 – -0.268 -1.623 –
Donor et al. 2020 77.787 45.715 – -0.33 -1.77 20.8
Cantat-Gaudin & Anders 2020 77.786 45.718 0.252 -0.265 -1.628 –
Bossini et al. 2019 77.786 45.718 – – – –
Soubiran et al. 2018 77.786 45.718 – – – 11.18
Bica et al. 2019 77.785 45.721 – – – –
Cantat-Gaudin et al. 2018 77.786 45.718 0.252 -0.265 -1.628 –
Dias et al. 2014 77.792 45.713 – 3.21 -1.74 –
Glushkova et al. 2010 77.781 45.719 – – – –
Froebrich et al. 2007 77.792 45.713 – – – –
Dias et al. 2002 77.792 45.713 – 3.21 -1.74 –

πŸ’‘ 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
Li et al. 2025 3.53 1.21 – 1024 -0.363 – – –
Hu & Soubiran 2025 – – – – -0.270* – – –
Almeida et al. 2025 3.51 1.30 – 1021 – 637 – –
Zhang et al. 2024 – – – – -0.197* – – –
Hunt & Reffert 2024 – – – – – 840* – –
Cavallo et al. 2024 2.79 1.05 – 1514 -0.360 – – –
Hunt & Reffert 2023 3.60 0.72 0.92 897 – – – –
Almeida et al. 2023 3.36 1.15 – 1222 -0.262 513* 0.73 –
Dias et al. 2021 3.51 1.30 – 1021 -0.319 – – –
Cantat-Gaudin et al. 2020 3.58 0.86 – 871 – – – –
Donor et al. 2020 – – – – -0.400 – – –
Cantat-Gaudin & Anders 2020 3.56 – – – – – – –
Bossini et al. 2019 4.25 1.06 – 738 0.000 – – –
Soubiran et al. 2018 3.56 – – – – – – –
Cantat-Gaudin et al. 2018 3.56 – – – – – – –
Glushkova et al. 2010 3.40 0.74 – 891 – – – –
Dias et al. 2002 4.50 1.29 – 638 – – – –

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

Visualization
ℹ️
FSR 0716 UCC
FSR 0716 HUNT23
FSR 0716 CANTAT20
Galactocentric position diagram