ASCC 33

(MWSC 1077)

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0.27 UTI
0.0
CN
0.1
Cdens
0.25
CC3
0.5
Clit
1.0
Cdup
Stellar density (N50/rad) 0.5 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.1 Very loose
  • CC3 0.25 Low quality
  • Clit 0.5 Moderately studied
  • Cdup 1.0 Unique

Overview

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ASCC 33 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very close* distance, near the mid-plane, affected by low extinction. It is catalogued as a very massive, near-solar metallicity, very young cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~0.43 kpc) differs significantly from the median photometric distance (~0.80 kpc).

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 105.204 -24.442 2.321 -9.887 1.192 17.282
Cavallo et al. 2024 104.696 -24.009 2.358 – – –
Hunt & Reffert 2023 105.454 -24.437 2.324 -9.781 1.143 16.879
Bica et al. 2019 105.797 -25.054 – – – –
Dias et al. 2014 105.796 -25.05 – -1.86 0.22 –
Gozha et al. 2012 105.796 -25.05 – – – –
Piskunov et al. 2008 105.792 -25.045 – – – –
Kharchenko et al. 2007 105.79 -25.05 – 0.9 – 15.0
Kharchenko et al. 2005 105.79 -25.05 – -3.78 3.78 15.0
Dias et al. 2002 105.796 -25.05 – -3.78 3.78 16.15

💡 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– 0.8 0.16 0.37 18 -0.018 7762 – –
Cavallo et al. 2024 0.43 0.44 – 89 0.130 – – –
Hunt & Reffert 2023 0.41 0.06 0.37 215 – – – –
Gozha et al. 2012 0.80 – – 18 – 7762 – –
Piskunov et al. 2008 0.80 0.16 – 18 – – – –
Kharchenko et al. 2005 0.80 0.16 – 18 – – – –
Dias et al. 2002 0.80 0.16 – 18 -0.166 – – –

Visualization

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