ASCC 56

(MWSC 1772)

Click to load Aladin Lite
0.25 UTI
0.0
CN
0.04
Cdens
0.12
CC3
0.55
Clit
1.0
Cdup
Radius (P>50% members) 7.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.04 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.55 Moderately studied
  • Cdup 1.0 Unique

Overview

â„šī¸
ASCC 56 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 low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~4.03 kpc) differs significantly from the median photometric distance (~0.80 kpc).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 152.062 -64.382 0.248 -6.025 2.777 35.684
Just et al. 2023 152.072 -64.377 – – – –
Bica et al. 2019 152.063 -64.365 – – – –
Kharchenko et al. 2016 152.072 -64.377 – – – –
Dias et al. 2014 152.054 -64.37 – -7.29 4.15 –
Kharchenko et al. 2013 152.077 -64.38 – -8.52 0.9 –
Piskunov et al. 2008 152.063 -64.365 – – – –
Piskunov et al. 2007 152.063 -64.365 – – – –
Kharchenko et al. 2005 152.05 -64.37 – -7.61 3.57 –
Dias et al. 2002 152.054 -64.37 – -7.29 4.15 –

💡 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 0.34 – 120 – 118 – –
Just et al. 2023 – – – 432 – 68 – –
Kharchenko et al. 2016 0.80 0.42 – 432 – – – –
Kharchenko et al. 2013 0.80 0.42 – 432 – – – –
Piskunov et al. 2008 0.80 0.34 – 120 – 406(1) – –
Piskunov et al. 2007 0.80 0.34 – 120 – 118 – –
Kharchenko et al. 2005 0.80 0.34 – 120 – – – –
Dias et al. 2002 0.80 0.34 – 120 – – – –

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

Visualization

â„šī¸