Lynga 15

(MWSC 1965)

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0.58 UTI
0.52
CN
0.65
Cdens
0.75
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members) 7.9 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 0.65 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.5 Moderately studied
  • Cdup 1.0 Unique

Overview

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Lynga 15 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is moderately studied in the literature.
Relatively close Moderate extinction Near-solar metallicity Young

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 – 175.494 -62.467 0.571 -6.483 0.869 -12.257
Hunt & Reffert 2024 175.487 -62.494 0.563 -6.488 0.869 -12.256
Cavallo et al. 2024 175.502 -62.49 0.567 – – –
Hunt & Reffert 2023 175.487 -62.494 0.563 -6.488 0.869 -12.256
Just et al. 2023 175.551 -62.507 – – – –
Kharchenko et al. 2016 175.551 -62.507 – – – –
Dias et al. 2014 175.6 -62.483 – -4.02 -6.47 –
Kharchenko et al. 2013 175.56 -62.51 – -4.97 -1.21 -8.2
Dias et al. 2002 175.6 -62.483 – -4.02 -6.47 -8.2

💡 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
Hunt & Reffert 2024 – – – – – 254* – –
Cavallo et al. 2024 1.45 0.53 – 355 0.110 – – –
Hunt & Reffert 2023 1.63 0.82 1.33 93 – – – –
Just et al. 2023 – – – 25 – 38 – –
Kharchenko et al. 2016 1.38 1.94 – 25 – – – –
Kharchenko et al. 2013 1.38 1.94 – 25 – – – –
Dias et al. 2002 1.38 1.94 – 25 – – – –

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

Visualization

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