Loden 402

(MWSC 1954)

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0.27 UTI
0.0
CN
0.01
Cdens
0.12
CC3
0.6
Clit
1.0
Cdup
Radius (P>50% members) 8.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.01 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.6 Moderately studied
  • Cdup 1.0 Unique

Overview

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Loden 402 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by low extinction. It is catalogued as a massive, intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~5.27 kpc) differs significantly from the median photometric distance (~2.45 kpc).

Relatively close Low extinction Massive 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 – 173.189 -60.682 0.19 -6.286 1.719 -11.389
Just et al. 2023 173.077 -60.702 – – – –
Bica et al. 2019 173.161 -60.711 – – – –
Kharchenko et al. 2016 173.077 -60.702 – – – –
Dias et al. 2014 173.217 -60.717 – -3.23 -3.59 –
Kharchenko et al. 2013 173.085 -60.705 – -7.4 0.9 -3.0
Gozha et al. 2012 173.217 -60.717 – – – –
Piskunov et al. 2008 173.161 -60.711 – – – –
Kharchenko et al. 2007 173.22 -60.72 – 0.15 – -3.0
Kharchenko et al. 2005 173.17 -60.72 – -6.9 -0.53 –
Dias et al. 2002 173.217 -60.717 – -3.23 -3.59 -3.0

💡 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 – – – 251 – 268 – –
Kharchenko et al. 2016 1.51 0.97 – 251 – – – –
Kharchenko et al. 2013 1.51 0.97 – 251 – – – –
Gozha et al. 2012 2.45 – – 158 – 3311 – –
Piskunov et al. 2008 2.45 0.56 – 158 – – – –
Kharchenko et al. 2005 2.45 0.56 – 158 – – – –
Dias et al. 2002 2.45 0.56 – 158 – – – –

Visualization

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