ASCC 54

(MWSC 1709)

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0.24 UTI
0.0
CN
0.04
Cdens
0.25
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad) 0.2 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.04 Very loose
  • CC3 0.25 Low quality
  • Clit 0.45 Poorly studied
  • Cdup 1.0 Unique

Overview

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ASCC 54 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 an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.64 kpc) differs significantly from the median photometric distance (~1.20 kpc).

Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 146.191 -54.427 0.275 -4.864 3.415 9.809
Just et al. 2023 146.192 -54.431 – – – –
Bica et al. 2019 146.229 -54.44 – – – –
Kharchenko et al. 2016 146.192 -54.431 – – – –
Dias et al. 2014 146.192 -54.44 – -3.73 0.14 –
Kharchenko et al. 2013 146.197 -54.435 – -8.17 1.75 –
Piskunov et al. 2008 146.191 -54.435 – – – –
Kharchenko et al. 2005 146.19 -54.44 – -7.73 1.08 –
Dias et al. 2002 146.192 -54.44 – -7.73 1.08 –

💡 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– 1.2 0.16 – 712 – 284 – –
Just et al. 2023 – – – 733 – 284 – –
Kharchenko et al. 2016 1.75 0.32 – 733 – – – –
Kharchenko et al. 2013 1.75 0.32 – 733 – – – –
Piskunov et al. 2008 1.20 0.16 – 692 – – – –
Kharchenko et al. 2005 1.20 0.16 – 692 – – – –
Dias et al. 2002 1.20 0.16 – 692 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1837 24.0 146.09 -54.67 0.33 -4.91 3.43 6.08 0.09

💡 Note: The % column shows the percentage of members that ASCC 54 shares with each listed object.

Visualization

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