ASCC 40

(MWSC 1266)

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0.36 UTI
0.26
CN
0.02
Cdens
0.62
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad) 0.1 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 0.02 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.45 Poorly studied
  • Cdup 1.0 Unique

Overview

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ASCC 40 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a large* distance, above 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 (~5.51 kpc) differs significantly from the median photometric distance (~0.70 kpc).

Note: This object shares a moderate percentage of members with 2 later reported entries. 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– 113.43 -13.765 0.182 -1.378 1.741 95.095
Just et al. 2023 113.408 -13.763 – – – –
Bica et al. 2019 113.401 -13.755 – – – –
Kharchenko et al. 2016 113.408 -13.763 – – – –
Dias et al. 2014 113.4 -13.76 – -2.47 1.72 –
Kharchenko et al. 2013 113.415 -13.765 – -1.13 -1.12 –
Piskunov et al. 2008 113.391 -13.76 – – – –
Kharchenko et al. 2005 113.4 -13.76 – -2.07 2.7 –
Dias et al. 2002 113.4 -13.76 – -2.47 1.72 –

💡 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– 0.7 0.34 – 506 – 630 – –
Just et al. 2023 – – – 631 – 630 – –
Kharchenko et al. 2016 3.11 1.29 – 631 – – – –
Kharchenko et al. 2013 3.11 1.29 – 631 – – – –
Piskunov et al. 2008 0.70 0.34 – 380 – – – –
Kharchenko et al. 2005 0.70 0.34 – 380 – – – –
Dias et al. 2002 0.70 0.34 – 380 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3444 34.6 113.59 -13.65 0.2 -1.37 1.87 77.28 0.03
HSC 1814 34.6 113.52 -13.61 0.2 -1.37 1.87 90.31 0.1

💡 Note: The % column shows the percentage of members that ASCC 40 shares with each listed object.

Visualization

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