ESO 494 09

(MWSC 1400)

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0.64 UTI
0.29
CN
1.0
Cdens
0.62
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members) 2.5 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.65 Moderately studied
  • Cdup 1.0 Unique

Overview

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ESO 494 09 is a poorly populated, very dense 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, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~2.97 kpc) differs significantly from the median photometric distance (~2.06 kpc).

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 Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 119.738 -27.661 0.337 -2.562 3.79 36.926
Hu & Soubiran 2025 119.71 -27.645 – – – –
Hunt & Reffert 2024 119.726 -27.673 0.341 -2.563 3.806 36.864
Cavallo et al. 2024 119.71 -27.645 0.34 – – –
Hunt & Reffert 2023 119.726 -27.673 0.341 -2.563 3.806 36.864
Just et al. 2023 119.811 -27.581 – – – –
Bica et al. 2019 119.811 -27.584 – – – –
Loktin & Popova 2017 119.82 -27.582 – -1.557 2.311 –
Kharchenko et al. 2016 119.811 -27.581 – – – –
Dias et al. 2014 119.817 -27.585 – -1.77 3.51 –
Kharchenko et al. 2013 119.817 -27.583 – -2.62 1.0 –
Dias et al. 2002 119.817 -27.585 – -1.78 3.5 –

💡 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
Hu & Soubiran 2025 – – – – -0.120* – – –
Hunt & Reffert 2024 – – – – – 337* – –
Cavallo et al. 2024 2.83 1.51 – 589 0.430 – – –
Hunt & Reffert 2023 2.78 1.39 1.20 619 – – – –
Just et al. 2023 – – – 543 – 107 – –
Loktin & Popova 2017 2.21 0.70 – 977 – – – –
Kharchenko et al. 2016 1.91 0.97 – 543 – – – –
Kharchenko et al. 2013 1.91 0.97 – 543 – – – –
Dias et al. 2002 1.21 1.30 – 63 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1402 86.2 119.72 -27.66 0.34 -2.56 3.8 37.53 0.13

💡 Note: The % column shows the percentage of members that ESO 494 09 shares with each listed object.

Visualization

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