Loden 309

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0.38 UTI
0.39
CN
0.18
Cdens
0.25
CC3
0.55
Clit
1.0
Cdup
Radius (P>50% members) 11.5 [arcmin]
  • CN 0.39 Poorly populated
  • Cdens 0.18 Very loose
  • CC3 0.25 Low quality
  • Clit 0.55 Moderately studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Loden 309 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a relatively close* distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~1.96 kpc) differs significantly from the median photometric distance (~0.80 kpc).

Close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 167.446 -60.56 0.51 -9.239 2.351 -49.436
Hu & Soubiran 2025 167.821 -60.532 – – – –
Hunt & Reffert 2024 167.369 -60.484 0.514 -9.25 2.33 -49.375
Cavallo et al. 2024 167.821 -60.532 0.513 – – –
Hunt & Reffert 2023 167.369 -60.484 0.514 -9.25 2.33 -49.375
Dias et al. 2014 167.679 -60.383 – -5.7 0.47 1.0
Piskunov et al. 2008 167.398 -60.578 – – – –
Kharchenko et al. 2005 167.41 -60.58 – -11.1 1.85 –
Kharchenko et al. 2003 167.43 -60.57 – -11.12 1.16 –
Dias et al. 2002 167.679 -60.383 – -5.7 0.47 1.0

💡 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
Hu & Soubiran 2025 – – – – -0.170* – – –
Hunt & Reffert 2024 – – – – – 54* – –
Cavallo et al. 2024 2.13 1.45 – 661 0.120 – – –
Hunt & Reffert 2023 1.81 1.27 1.14 282 – – – –
Piskunov et al. 2008 0.60 0.78 – 427 – – – –
Kharchenko et al. 2005 0.60 0.78 – 427 – – – –
Kharchenko et al. 2003 1.00 0.62 – – – – – –
Dias et al. 2002 0.60 0.78 – 427 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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