ESO 165 09

(MWSC 1625)

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0.25 UTI
0.0
CN
0.01
Cdens
0.12
CC3
0.55
Clit
1.0
Cdup
Radius (P>50% members) 7.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.01 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.55 Moderately studied
  • Cdup 1.0 Unique

Overview

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ESO 165 09 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large* distance, well below the mid-plane, affected by low extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~6.54 kpc) differs significantly from the median photometric distance (~0.45 kpc).

Very close Low extinction Low mass Intermediate age

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 136.31 -55.953 0.153 -3.203 3.596 –
Just et al. 2023 136.346 -55.935 – – – –
Bica et al. 2019 136.31 -55.952 – – – –
Loktin & Popova 2017 136.305 -55.955 – -10.15 10.47 –
Kharchenko et al. 2016 136.346 -55.935 – – – –
Dias et al. 2014 136.312 -55.955 – -2.99 5.85 –
Kharchenko et al. 2013 136.35 -55.938 – -9.83 10.62 –
Piskunov et al. 2008 136.297 -55.958 – – – –
Kharchenko et al. 2005 136.3 -55.96 – -10.15 10.47 –
Dias et al. 2002 136.312 -55.955 – -10.15 10.47 –

💡 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 – – – 822 – 16 – –
Loktin & Popova 2017 0.39 0.16 – 912 – – – –
Kharchenko et al. 2016 0.66 0.16 – 822 – – – –
Kharchenko et al. 2013 0.66 0.16 – 822 – – – –
Piskunov et al. 2008 0.45 0.16 – 912 – – – –
Kharchenko et al. 2005 0.45 0.16 – 912 – – – –
Dias et al. 2002 0.45 0.16 – 912 – – – –

Visualization

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