ASCC 115

(MWSC 3575)

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0.90 UTI
0.75
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members) 17.9 [arcmin]
  • CN 0.75 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique

Overview

ASCC 115 is a rich, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (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.

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 329.264 51.525 1.295 -0.55 -0.654 -15.515
Almeida et al. 2025 329.315 51.524
Alfonso et al. 2024 329.232 51.51 1.277 -0.55 -0.678
Hunt & Reffert 2024 329.19 51.549 1.287 -0.577 -0.677 -16.736
Cavallo et al. 2024 329.19 51.462 1.291
Hunt & Reffert 2023 329.19 51.549 1.287 -0.577 -0.677 -16.736
Just et al. 2023 329.161 51.521
He et al. 2022 329.172 51.541 1.308 -0.553 -0.629
Tarricq et al. 2022 329.316 51.56 1.303 -0.512 -0.619
Dias et al. 2021 329.315 51.524 1.313 -0.549 -0.551
Cantat-Gaudin et al. 2020 329.28 51.558 1.311 -0.549 -0.543
Bossini et al. 2019 329.28 51.558
Soubiran et al. 2018 329.28 51.558 -46.01
Bica et al. 2019 329.217 51.482
Cantat-Gaudin et al. 2018 329.28 51.558 1.311 -0.549 -0.543
Kharchenko et al. 2016 329.161 51.521
Kharchenko et al. 2013 329.167 51.525 0.4 -0.83 -9.0
Kharchenko et al. 2012 329.167 51.525 0.4 -0.83 -9.0
Piskunov et al. 2008 329.217 51.482
Kharchenko et al. 2007 329.22 51.48 0.16 -9.0
Kharchenko et al. 2005 329.22 51.48 0.15 -1.28 -9.0
Dias et al. 2002 329.221 51.48 0.27 -1.29 -9.0

💡 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 0.74 0.94 245 102
Alfonso et al. 2024 0.73 0.72 196 0.050
Hunt & Reffert 2024 198*
Cavallo et al. 2024 0.81 1.05 126 0.200
Hunt & Reffert 2023 0.73 0.80 0.90 78
Just et al. 2023 224 29
He et al. 2022 1.05 112
Tarricq et al. 2022 0.72 138
Dias et al. 2021 0.74 0.94 245 0.050
Cantat-Gaudin et al. 2020 0.73 0.72 132
Bossini et al. 2019 0.71 0.63 105 0.000
Soubiran et al. 2018 0.75
Cantat-Gaudin et al. 2018 0.75
Kharchenko et al. 2016 0.75 0.46 224
Kharchenko et al. 2013 0.75 0.46 224
Kharchenko et al. 2012 0.75 0.46 224
Piskunov et al. 2008 0.60 0.46 389
Kharchenko et al. 2005 0.60 0.46 389
Dias et al. 2002 0.60 0.46 389

💡 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.