Loden 1

(MWSC 1758)

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0.17 UTI
0.0
CN
0.02
Cdens
0.25
CC3
0.29
Clit
1.0
Cdup
Core radius and density 1.9 [pc], 0.09 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.02 Very loose
  • CC3 0.25 Low quality
  • Clit 0.29 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Loden 1 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by low extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~2.70 kpc) differs significantly from the median photometric distance (~0.79 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.

Cantat-Gaudin & Anders (2020)
Initially proposed as an old nearby cluster, but radial velocity studies show no co-moving group; not physical. More details in Appendix A of the article.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 151.268 -55.768 0.37 -6.622 4.295 7.591
Just et al. 2023 151.302 -55.802 – – – –
Dias et al. 2018 – – – -5.46 2.32 –
Dib et al. 2018 151.308 -55.805 – – – –
Sampedro et al. 2017 151.262 -55.8 – -8.41 0.78 –
Joshi et al. 2016 151.308 -55.805 – – – –
Kharchenko et al. 2016 151.302 -55.802 – – – –
Dias et al. 2014 151.262 -55.8 – -8.3 1.04 –
Kharchenko et al. 2013 151.308 -55.805 – -9.49 4.55 –
Piskunov et al. 2008 151.265 -55.796 – – – –
Kharchenko et al. 2005 151.26 -55.8 – -10.37 4.18 –

💡 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– 0.79 0.7 – 200 – 5 – –
Just et al. 2023 – – – 200 – 3 – –
Dib et al. 2018 0.79 – – 200 – – – –
Joshi et al. 2016 0.79 0.70 – 200 – 7 – –
Kharchenko et al. 2016 0.79 0.70 – 200 – – – –
Kharchenko et al. 2013 0.79 0.70 – 200 – – – –
Piskunov et al. 2008 0.36 0.32 – 1950 – – – –
Kharchenko et al. 2005 0.36 0.32 – 1950 – – – –

Visualization

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