Westerlund 2

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0.77 UTI
0.79
CN
1.0
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members) 0.9 [arcmin]
  • CN 0.79 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.65 Moderately studied
  • Cdup 1.0 Unique

Overview

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Westerlund 2 is a rich, very dense object of high C3 quality. Its parallax locates it at a large* distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~5.09 kpc) differs significantly from the median photometric distance (~2.85 kpc).

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

Relatively close High extinction Massive Metal-rich Very young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 156.01 -57.758 0.197 -5.32 2.871 68.86
Hunt & Reffert 2024 156.003 -57.756 0.192 -5.352 2.879 –
Celli et al. 2024 155.992 -57.764 – – – –
Cavallo et al. 2024 156.008 -57.756 0.192 – – –
Hunt & Reffert 2023 156.003 -57.756 0.192 -5.352 2.879 –
Cantat-Gaudin et al. 2020 156.01 -57.758 0.209 -5.246 2.895 –
Cantat-Gaudin & Anders 2020 156.01 -57.758 0.209 -5.246 2.895 –
Cantat-Gaudin et al. 2018 156.01 -57.758 0.209 -5.246 2.895 –
Loktin & Popova 2017 156.015 -57.767 – -7.5 4.22 –
Dias et al. 2014 156.008 -57.767 – -0.89 2.45 –
van den Bergh 2006 155.992 -57.764 – – – –
Dias et al. 2002 156.008 -57.767 – -6.77 4.84 –

💡 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
Hunt & Reffert 2024 – – – – – 2390* – –
Celli et al. 2024 – – – 4 – 2172 – –
Cavallo et al. 2024 1.86 4.46 – 174 0.760 – – –
Hunt & Reffert 2023 5.41 4.52 3.03 76 – – – –
Cantat-Gaudin & Anders 2020 4.21 – – – – – – –
Cantat-Gaudin et al. 2018 4.21 – – – – – – –
Loktin & Popova 2017 1.92 2.32 – 21 – – – –
van den Bergh 2006 1.87 2.42 – 17 – – – –
Dias et al. 2002 2.85 5.12 – 2 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Bica 417 78.8 156.01 -57.76 0.19 -5.35 2.86 – 0.03

💡 Note: The % column shows the percentage of members that Westerlund 2 shares with each listed object.

Visualization

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