ASCC 17

(MWSC 534)

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0.29 UTI
0.0
CN
0.07
Cdens
0.12
CC3
0.62
Clit
1.0
Cdup
Stellar density (N50/rad) 0.3 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.07 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.62 Moderately studied
  • Cdup 1.0 Unique

Overview

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ASCC 17 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 massive, very young cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~4.41 kpc) differs significantly from the median photometric distance (~2.00 kpc).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 81.328 30.116 0.227 0.099 -0.364 12.568
Just et al. 2023 81.321 30.183 – – – –
Bica et al. 2019 81.3 30.173 – – – –
Kharchenko et al. 2016 81.321 30.183 – – – –
Dias et al. 2014 81.3 30.17 – 2.55 -3.74 –
Kharchenko et al. 2013 81.33 30.182 – 2.57 -3.15 -16.0
Gozha et al. 2012 81.3 30.17 – – – –
Kharchenko et al. 2012 81.33 30.182 – 2.57 -3.15 -16.0
Piskunov et al. 2008 81.29 30.167 – – – –
Kharchenko et al. 2007 81.3 30.17 – 0.25 – -16.0
Kharchenko et al. 2005 81.3 30.17 – 1.33 -6.39 -16.0
Dias et al. 2002 81.3 30.17 – 2.55 -3.74 -16.0

💡 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] Bfrac BSS
UCC 99999– 2.0 1.07 – 16 – 1391 – –
Just et al. 2023 – – – 18 – 327 – –
Kharchenko et al. 2016 1.85 1.15 – 18 – – – –
Kharchenko et al. 2013 1.85 1.15 – 18 – – – –
Gozha et al. 2012 2.00 – – 13 – 2455 – –
Kharchenko et al. 2012 1.85 1.15 – 18 – – – –
Piskunov et al. 2008 2.00 0.99 – 13 – – – –
Kharchenko et al. 2005 2.00 0.99 – 13 – – – –
Dias et al. 2002 2.00 0.99 – 13 – – – –

Visualization

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