Berkeley 49

(FSR 0191; MWSC 3216; OCL 144)

Click to load Aladin Lite
0.84 UTI
0.78
CN
1.0
Cdens
0.75
CC3
0.84
Clit
1.0
Cdup
N50 (P>50% members) 183
Stellar density (N50/rad) 84.7 [N/pc2]
C3 classification AB
  • CN 0.78 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.84 Well-studied
  • Cdup 1.0 Unique
πŸ“₯ Members πŸ“Š Colab πŸ”¬ Bayestar19 MOCAMOCA πŸ” CDS πŸ” Simbad πŸ” CDS (Ξ±, Ξ΄) πŸ” Simbad (Ξ±, Ξ΄)

Overview
ℹ️
Berkeley 49 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.

Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.

Cavallo et al. (2024)
Silver sample.

Data
πŸ” Search references for Berkeley 49 in: SciX Simbad
ℹ️
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 299.867 34.643 0.297 -3.016 -6.085 -14.8
Hunt & Reffert 2024 299.869 34.643 0.303 -3.024 -6.082 -20.271
Cavallo et al. 2024 299.868 34.629 0.306 – – –
Hunt & Reffert 2023 299.869 34.643 0.303 -3.024 -6.082 -20.271
Just et al. 2023 299.867 34.642 – – – –
Cantat-Gaudin et al. 2020 299.872 34.643 0.286 -2.995 -6.095 –
SΓ‘nchez et al. 2020 299.875 34.642 – -3.009 -6.146 –
Cantat-Gaudin & Anders 2020 299.872 34.643 0.286 -2.995 -6.095 –
Soubiran et al. 2018 299.872 34.643 – – – -13.19
Bica et al. 2019 299.871 34.645 – – – –
Cantat-Gaudin et al. 2018 299.872 34.643 0.286 -2.995 -6.095 –
Loktin & Popova 2017 299.865 34.652 – -3.888 -3.645 –
Kharchenko et al. 2016 299.867 34.642 – – – –
Dias et al. 2014 299.875 34.642 – -0.83 -8.02 –
Kharchenko et al. 2013 299.872 34.645 – -2.9 -3.3 –
Froebrich et al. 2007 299.871 34.656 – – – –
Dias et al. 2002 299.875 34.642 – -2.9 -3.3 –

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] Bfrac BSS
UCC 99999– 3.1 3.81 2.7 288 0.090 1073 – –
Hunt & Reffert 2024 – – – – – 2008(1) – –
Cavallo et al. 2024 3.37 4.22 – 63 0.090 – – –
Hunt & Reffert 2023 2.96 4.12 2.70 110 – – – –
Just et al. 2023 – – – 288 – 138 – –
Cantat-Gaudin et al. 2020 3.03 3.24 – 257 – – – –
Cantat-Gaudin & Anders 2020 3.17 – – – – – – –
Soubiran et al. 2018 3.17 – – – – – – –
Cantat-Gaudin et al. 2018 3.17 – – – – – – –
Loktin & Popova 2017 3.78 3.28 – 513 – – – –
Kharchenko et al. 2016 2.30 3.81 – 288 – – – –
Kharchenko et al. 2013 2.30 3.81 – 288 – – – –
Dias et al. 2002 2.09 3.66 – 794 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Teutsch J2000.5+3432 1.1 300.14 34.54 0.24 -2.61 -6.31 -28.5 0.24

πŸ’‘ Note: The % column shows the percentage of members that Berkeley 49 shares with each listed object.

Visualization
ℹ️
Berkeley 49 UCC
Berkeley 49 HUNT23
Berkeley 49 CANTAT20
Galactocentric position diagram