ESO 435 09

(MWSC 1728)

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0.09 UTI
0.0
CN
0.04
Cdens
0.12
CC3
0.13
Clit
1.0
Cdup
Core radius and density 2.5 [pc], 0.2 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.04 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.13 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
ESO 435 09 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, well above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 148.956 -29.008 0.451 -7.767 2.899 73.757
Just et al. 2023 148.861 -28.962 – – – –
Sampedro et al. 2017 148.887 -28.987 – -3.61 0.09 –
Kharchenko et al. 2016 148.861 -28.962 – – – –
Dias et al. 2014 148.888 -28.987 – -5.12 1.34 –
Kharchenko et al. 2013 148.867 -28.965 – -4.29 0.87 –
Dias et al. 2002 148.887 -28.987 – -5.16 1.41 –

💡 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– 2.25 2.3 – 266 – 601 – –
Just et al. 2023 – – – 266 – 601 – –
Kharchenko et al. 2016 2.25 2.30 – 266 – – – –
Kharchenko et al. 2013 2.25 2.30 – 266 – – – –
Dias et al. 2002 2.25 2.30 – 266 – – – –

Visualization

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