ASCC 64

(MWSC 1884)

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0.32 UTI
0.0
CN
0.04
Cdens
0.38
CC3
0.6
Clit
1.0
Cdup
Radius (P>50% members) 7.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.04 Very loose
  • CC3 0.38 Low quality
  • Clit 0.6 Moderately studied
  • Cdup 1.0 Unique

Overview

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ASCC 64 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by low extinction. It is catalogued as a young cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~4.31 kpc) differs significantly from the median photometric distance (~1.50 kpc).

Relatively close Low extinction Young

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 165.777 -60.911 0.232 -6.126 2.015 12.074
Just et al. 2023 165.758 -60.911 – – – –
Bica et al. 2019 165.761 -60.921 – – – –
Kharchenko et al. 2016 165.758 -60.911 – – – –
Dias et al. 2014 165.767 -60.92 – -2.94 -3.58 –
Kharchenko et al. 2013 165.765 -60.915 – -5.6 1.77 1.4
Gozha et al. 2012 165.767 -60.92 – – – –
Piskunov et al. 2008 165.761 -60.921 – – – –
Kharchenko et al. 2007 165.76 -60.92 – 0.18 – -8.33
Kharchenko et al. 2005 165.76 -60.92 – -5.88 1.44 -8.33
Dias et al. 2002 165.767 -60.92 – -2.94 -3.58 1.15

💡 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] Bfr BSS
Just et al. 2023 – – – 126 – 449 – –
Kharchenko et al. 2016 1.70 0.46 – 126 – – – –
Kharchenko et al. 2013 1.70 0.46 – 126 – – – –
Gozha et al. 2012 1.50 – – 83 – 617 – –
Piskunov et al. 2008 1.50 0.46 – 83 – – – –
Kharchenko et al. 2005 1.50 0.46 – 83 – – – –
Dias et al. 2002 1.50 0.46 – 83 – – – –

Visualization

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