IC 2156

(MWSC 723)

Click to load Aladin Lite
0.46 UTI
0.32
CN
0.46
Cdens
0.5
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members) 4.8 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 0.46 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.5 Moderately studied
  • Cdup 1.0 Unique

Overview

â„šī¸
IC 2156 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is moderately studied in the literature.

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

Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 91.244 24.141 0.375 0.765 -2.413 59.864
Zhang et al. 2024 91.228 24.146 – – – –
Hunt & Reffert 2024 91.228 24.146 0.378 0.781 -2.415 –
Cavallo et al. 2024 91.248 24.143 0.377 – – –
Hunt & Reffert 2023 91.228 24.146 0.378 0.781 -2.415 –
Bica et al. 2019 91.21 24.082 – – – –
Loktin & Popova 2017 91.215 24.158 – -0.031 -0.555 –
Dias et al. 2014 91.213 24.158 – -1.96 -2.51 –
Dias et al. 2002 91.213 24.158 – -1.96 -2.51 –

💡 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
Zhang et al. 2024 – – – – -0.158* – – –
Hunt & Reffert 2024 – – – – – 264* – –
Cavallo et al. 2024 2.79 1.66 – 46 0.240 – – –
Hunt & Reffert 2023 2.49 1.56 0.46 29 – – – –
Loktin & Popova 2017 3.63 1.76 – 4 – – – –
Dias et al. 2002 2.10 2.08 – 251 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1302 90.6 91.24 24.14 0.38 0.76 -2.41 – 0.0

💡 Note: The % column shows the percentage of members that IC 2156 shares with each listed object.

Visualization

â„šī¸