King 21

(OCL 270; MWSC 3762)

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C3
N_50
r_50
AB 184 2.0
Summary

King 21 is a rich, very dense object of high C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is well-studied in the literature.

This object shares a small percentage of members with 2 later reported entries.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 357.475 62.717 0.72 0.77
Kharchenko et al. (2012) 357.465 62.7 -2.33 -4.11
Loktin & Popova (2017) 357.48 62.718 -1.051 -4.543
Cantat-Gaudin et al. (2018) 357.479 62.705 0.305 -3.259 -1.675
Bica et al. (2019) 357.447 62.701
Cantat-Gaudin et al. (2020) 357.479 62.705 0.305 -3.259 -1.675
Dias et al. (2021) 357.473 62.707 0.307 -3.257 -1.661
Hunt & Reffert (2023) 357.477 62.7 0.319 -3.231 -1.717 -78.265
Cavallo et al. (2024) 357.494 62.708 0.319
Hunt & Reffert (2024) 357.477 62.7 0.319 -3.231 -1.717 -78.265
Almeida et al. (2025) 357.473 62.707
           
UCC 357.485 62.704 0.317 -3.238 -1.713 -78.273
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Explore data in Colab

Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.886, Dist=2103.0, Age=7.163, [Fe/H]=0.06
Kharchenko et al. (2012) e_bv=0.799, distance=2101, log_age=7.8
Loktin & Popova (2017) E(B-V)=0.856, Dist=2128, logt=7.213
Cantat-Gaudin et al. (2018) dmode=2994.5
Cantat-Gaudin et al. (2020) AVNN=2.03, DistPc=3005.0, AgeNN=7.99
Dias et al. (2021) Av=2.377, Dist=2591, logage=7.668, [Fe/H]=0.028
Hunt & Reffert (2023) AV50=2.557, diffAV50=1.579, MOD50=12.308, logAge50=7.72
Cavallo et al. (2024) AV50=2.62, dMod50=12.7, logAge50=7.75, [Fe/H]50=0.54
Hunt & Reffert (2024) MassJ=1532.77, MassTot=1532.77
Almeida et al. (2025) AV=2.377, Dist=2591, logAge=7.668, MassRk=632.4

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0212 13.6 357.48 62.71 0.34 -3.26 -1.7 0.0
CWWDL 10426 1.1 357.55 62.97 0.32 -3.04 -1.36 -89.18 0.11