ASCC 48

(MWSC 1506)

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0.28 UTI
0.0
CN
0.04
Cdens
0.12
CC3
0.62
Clit
1.0
Cdup
Stellar density (N50/rad) 0.2 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.04 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.62 Moderately studied
  • Cdup 1.0 Unique

Overview

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ASCC 48 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by low extinction. It is catalogued as a low-mass, old cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~5.09 kpc) differs significantly from the median photometric distance (~0.40 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– 128.602 -37.671 0.197 -3.031 3.303 69.29
Just et al. 2023 128.657 -37.627 – – – –
Bica et al. 2019 128.616 -37.61 – – – –
Kharchenko et al. 2016 128.657 -37.627 – – – –
Dias et al. 2014 128.625 -37.61 – -2.46 1.2 –
Kharchenko et al. 2013 128.662 -37.63 – -10.75 10.43 22.5
Gozha et al. 2012 128.625 -37.61 – – – –
Piskunov et al. 2008 128.616 -37.61 – – – –
Kharchenko et al. 2007 128.62 -37.61 – 0.32 – 22.5
Piskunov et al. 2007 128.616 -37.61 – – – –
Kharchenko et al. 2005 128.62 -37.61 – -11.63 10.72 22.5
Dias et al. 2002 128.625 -37.61 – -11.63 10.72 22.5

💡 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– 0.4 0.0 – 1230 – 26 – –
Just et al. 2023 – – – 1531 – 6 – –
Kharchenko et al. 2016 0.55 0.00 – 1531 – – – –
Kharchenko et al. 2013 0.55 0.00 – 1531 – – – –
Gozha et al. 2012 0.40 – – 1230 – 32 – –
Piskunov et al. 2008 0.40 0.00 – 1230 – 57(1) – –
Piskunov et al. 2007 0.40 0.00 – 1230 – 20 – –
Kharchenko et al. 2005 0.40 0.00 – 1230 – – – –
Dias et al. 2002 0.40 0.00 – 1230 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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