Loden 1375

(MWSC 2246; OCL 923.2)

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0.14 UTI
0.0
CN
0.05
Cdens
0.12
CC3
0.26
Clit
1.0
Cdup
Core radius and density 1.9 [pc], 0.2 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.05 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.26 Poorly studied
  • Cdup 1.0 Unique

Overview

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Loden 1375 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~4.37 kpc) differs significantly from the median photometric distance (~1.82 kpc).

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– 221.044 -63.385 0.229 -5.032 -4.14 -75.676
Just et al. 2023 221.072 -63.403 – – – –
Bica et al. 2019 220.967 -63.375 – – – –
Dias et al. 2018 – – – -6.34 -3.59 –
Dib et al. 2018 221.085 -63.405 – – – –
Sampedro et al. 2017 221.075 -63.417 – -8.87 -0.03 –
Kharchenko et al. 2016 221.072 -63.403 – – – –
Dias et al. 2014 221.075 -63.417 – -8.56 -0.35 –
Kharchenko et al. 2013 221.085 -63.405 – -6.87 -0.08 –
Dias et al. 2002 221.075 -63.417 – -8.56 -0.35 –
Lynga 1987 221.076 -63.385 – – – –

💡 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– 1.82 1.97 – 79 – 279 – –
Just et al. 2023 – – – 79 – 279 – –
Dib et al. 2018 1.82 – – 79 – – – –
Kharchenko et al. 2016 1.82 1.97 – 79 – – – –
Kharchenko et al. 2013 1.82 1.97 – 79 – – – –
Dias et al. 2002 1.82 1.97 – 79 – – – –

Visualization

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