IRAS 20306+4005

(MWSC 3361)

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0.15 UTI
0.64
CN
1.0
Cdens
1.0
CC3
0.13
Clit
0.25
Cdup
Core radius and density 0.6 [pc], 19 [pc-2]
  • CN 0.64 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.13 Rarely studied
  • Cdup 0.25 Possibly duplicate

Overview

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IRAS 20306+4005 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is rarely studied in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Palma et al. (2025)
Classified as tidal capture (resonant trapping pair) P296, along with CWNU_1243.

Cavallo et al. (2024)
Wood sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.25 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.25 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 308.049 40.292 1.023 -1.791 -4.003 –
Hunt & Reffert 2024 308.059 40.292 1.009 -1.811 -3.997 4.021
Cavallo et al. 2024 308.061 40.297 1.026 – – –
Hunt & Reffert 2023 308.059 40.292 1.009 -1.811 -3.997 4.021
Just et al. 2023 308.11 40.282 – – – –
Kharchenko et al. 2016 308.11 40.282 – – – –
Kharchenko et al. 2013 308.115 40.285 – 0.16 0.02 -9.8

💡 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– 1.27 3.7 2.51 4 -0.050 270 – –
Hunt & Reffert 2024 0.93 3.70 2.51 5 – 300(1) – –
Cavallo et al. 2024 1.27 2.86 – 5 -0.050 – – –
Hunt & Reffert 2023 0.93 3.70 2.51 5 – – – –
Just et al. 2023 – – – 3 – 240 – –
Kharchenko et al. 2016 2.02 4.60 – 3 – – – –
Kharchenko et al. 2013 2.02 4.60 – 3 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
DB2001 10 74.7 308.08 40.29 1.02 -1.8 -4.02 – 0.55
CWNU 1011 54.4 308.05 40.29 1.03 -1.66 -4.07 – 0.05

💡 Note: The % column shows the percentage of members that IRAS 20306+4005 shares with each listed object.

Visualization

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