FSR 0771

(MWSC 460)

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0.87 UTI
0.58
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members) 7.2 [arcmin]
  • CN 0.58 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique

Overview

FSR 0771 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is very well-studied in the literature.
Relatively close Moderate extinction Near-solar metallicity Intermediate age

Almeida et al. (2025): Mass determination: intermediate fit. Isochrone match: good fit.

Cavallo et al. (2024): Gold sample.

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 75.923 32.158 0.614 1.491 -4.254 -4.012
Almeida et al. 2025 75.902 32.164
Zhang et al. 2024 75.921 32.145
Hunt & Reffert 2024 75.921 32.145 0.611 1.498 -4.255 -6.513
Cavallo et al. 2024 75.927 32.133 0.61
Hunt & Reffert 2023 75.921 32.145 0.611 1.498 -4.255 -6.513
Just et al. 2023 75.935 32.165
Tarricq et al. 2022 75.917 32.178 0.584 1.484 -4.251
Dias et al. 2021 75.902 32.164 0.631 1.642 -4.214 -3.464
Cantat-Gaudin et al. 2020 75.919 32.157 0.618 1.631 -4.203
Bossini et al. 2019 75.919 32.157
Soubiran et al. 2018 75.919 32.157 -3.37
Bica et al. 2019 75.954 32.138
Cantat-Gaudin et al. 2018 75.919 32.157 0.618 1.631 -4.203
Kharchenko et al. 2016 75.935 32.165
Kharchenko et al. 2013 75.945 32.165 3.96 -5.49
Kharchenko et al. 2012 75.945 32.165 3.96 -5.49
Froebrich et al. 2007 75.946 32.142

💡 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
Almeida et al. 2025 1.44 2.19 301 226
Zhang et al. 2024 0.001*
Hunt & Reffert 2024 322*
Cavallo et al. 2024 1.51 2.11 372 0.310
Hunt & Reffert 2023 1.55 2.14 1.03 215
Just et al. 2023 327 86
Tarricq et al. 2022 1.47 309
Dias et al. 2021 1.44 2.19 301 0.099
Cantat-Gaudin et al. 2020 1.53 1.64 282
Bossini et al. 2019 1.86 2.02 157 0.000
Soubiran et al. 2018 1.55
Cantat-Gaudin et al. 2018 1.55
Kharchenko et al. 2016 1.71 2.33 327
Kharchenko et al. 2013 1.71 2.33 327
Kharchenko et al. 2012 1.71 2.33 327

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
(*): indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

Galactocentric position diagram

💡 Note: How are the galactocentric plots generated? See FAQ.