IRAS 20286+4105

(MWSC 3353)

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0.33 UTI
0.0
CN
0.63
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
C3 classification AA
Number of members (P>50%) 23
Radius (P>50% members) 5.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.63 Moderately dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
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IRAS 20286+4105 is a sparse, moderately dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high extinction. It is catalogued as a young cluster (see Parameters). It is rarely studied in the literature.
Relatively close High extinction Young

Data
🔍 Search references for IRAS 20286+4105 in: SciX Simbad
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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 307.582 41.24 0.58 -3.189 -4.316 –
Just et al. 2023 307.613 41.261 – – – –
Kharchenko et al. 2016 307.613 41.261 – – – –
Kharchenko et al. 2013 307.617 41.264 – 1.16 0.02 -17.4

💡 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
Just et al. 2023 – – – 89 – 103 – –
Kharchenko et al. 2016 1.86 3.36 – 89 – – – –
Kharchenko et al. 2013 1.86 3.36 – 89 – – – –

Visualization
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IRAS 20286+4105 UCC
Galactocentric position diagram