IRAS 06117+1901

(MWSC 816)

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0.56 UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.44
Clit
0.83
Cdup
C3 classification AB
Number of members (P>50%) 133
Radius (P>50% members) 8.1 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.44 Poorly studied
  • Cdup 0.83 Very likely unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
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IRAS 06117+1901 is a rich, very dense object of high 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, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data
🔍 Search references for IRAS 06117+1901 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 – 93.697 19.005 0.481 -0.069 -1.263 -5.101
Zhang et al. 2024 93.702 19.006 – – – –
Hunt & Reffert 2024 93.702 19.006 0.477 -0.064 -1.268 0.094
Cavallo et al. 2024 93.669 18.918 0.477 – – –
Hunt & Reffert 2023 93.702 19.006 0.477 -0.064 -1.268 0.094
Just et al. 2023 93.681 19.02 – – – –
Kharchenko et al. 2016 93.681 19.02 – – – –
Kharchenko et al. 2013 93.69 19.019 – 0.36 -5.16 –

💡 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 – – – – -0.183* – – –
Hunt & Reffert 2024 – – – – – 813* – –
Cavallo et al. 2024 1.93 1.67 – 16 0.080 – – –
Hunt & Reffert 2023 1.90 1.69 2.45 18 – – – –
Just et al. 2023 – – – 112 – 70 – –
Kharchenko et al. 2016 2.14 2.39 – 112 – – – –
Kharchenko et al. 2013 2.14 2.39 – 112 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0318 18.8 93.81 19.04 0.5 -0.06 -1.27 20.08 0.0
FSR 0909 17.3 93.87 19.04 0.48 -0.04 -1.26 20.08 0.4

💡 Note: The % column shows the percentage of members that IRAS 06117+1901 shares with each listed object.

Visualization
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IRAS 06117+1901 UCC
IRAS 06117+1901 HUNT23
Galactocentric position diagram