ASCC 11

(MWSC 284; Teutsch J0332.2+4450; FoF 2205)

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0.97 UTI
0.85
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members) 14.7 [arcmin]
  • CN 0.85 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique

Overview

ASCC 11 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low 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.
Close Low extinction Near-solar metallicity Intermediate age

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

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 53.044 44.848 1.171 0.909 -3.066 -16.549
Almeida et al. 2025 53.078 44.879
Alfonso et al. 2024 53.041 44.85 1.14 0.919 -3.075
Zhang et al. 2024 53.05 44.841
Hunt & Reffert 2024 53.05 44.841 1.171 0.905 -3.072 -17.285
Cavallo et al. 2024 53.054 44.844 1.172
Hunt & Reffert 2023 53.05 44.841 1.171 0.905 -3.072 -17.285
Just et al. 2023 53.059 44.839
He et al. 2022 53.043 44.843 1.173 0.912 -3.07
Tarricq et al. 2022 53.029 44.877 1.154 0.898 -3.067
Dias et al. 2021 53.078 44.879 1.142 0.95 -3.022 -14.242
Cantat-Gaudin et al. 2020 53.056 44.856 1.141 0.926 -3.03
Liu & Pang 2019 53.017 44.853 1.138 0.965 -3.013
Soubiran et al. 2018 53.056 44.856 -14.43
Bica et al. 2019 53.066 44.842
Cantat-Gaudin et al. 2018 53.056 44.856 1.141 0.926 -3.03
Kharchenko et al. 2016 53.059 44.839
Kharchenko et al. 2013 53.07 44.84 1.26 -4.75 0.7
Kharchenko et al. 2012 53.07 44.84 1.26 -4.75 0.73
Piskunov et al. 2008 53.058 44.834
Kharchenko et al. 2007 53.07 44.84 0.35 0.73
Kharchenko et al. 2005 53.07 44.84 0.15 -5.01 -3.45
Dias et al. 2002 53.071 44.84 1.26 -4.75 -3.24

💡 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 0.85 0.92 457 692
Alfonso et al. 2024 0.87 0.60 624 -0.055
Zhang et al. 2024 -0.266*
Hunt & Reffert 2024 688*
Cavallo et al. 2024 0.88 0.92 245 0.210
Hunt & Reffert 2023 0.80 0.73 1.00 234
Just et al. 2023 221 162
He et al. 2022 1.00 282
Tarricq et al. 2022 0.85 263
Dias et al. 2021 0.85 0.92 457 -0.056
Cantat-Gaudin et al. 2020 0.87 0.60 245
Liu & Pang 2019 100 0.500
Soubiran et al. 2018 0.85
Cantat-Gaudin et al. 2018 0.85
Kharchenko et al. 2016 0.84 0.84 221
Kharchenko et al. 2013 0.84 0.84 221
Kharchenko et al. 2012 0.84 0.84 221
Piskunov et al. 2008 0.65 0.46 407
Kharchenko et al. 2005 0.65 0.46 407
Dias et al. 2002 0.65 0.46 407

💡 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.