Dias 8

(MWSC 3195)

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0.11 UTI
0.0
CN
0.02
Cdens
0.12
CC3
0.19
Clit
1.0
Cdup
Core radius and density 4.1 [pc], 0.1 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.02 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.19 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Dias 8 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 old cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~3.44 kpc) differs significantly from the median photometric distance (~2.23 kpc).

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 298.011 11.611 0.291 -4.83 -6.338 –
Bica et al. 2019 298.035 11.634 – – – –
Dias et al. 2018 – – – -2.01 -3.77 –
Loktin & Popova 2017 298.035 11.628 – -1.054 -3.214 –
Sampedro et al. 2017 298.025 11.634 – -3.65 -3.39 –
Tadross 2014 298.029 11.632 – – – –
Dias et al. 2014 298.025 11.634 – -3.36 -3.03 –
Bukowiecki et al. 2011 298.046 11.626 – – – –
Dias et al. 2002 298.025 11.634 – -2.56 -3.28 –

💡 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– 2.235 0.95 – 2240 – – – –
Loktin & Popova 2017 2.25 0.20 – 6310 – – – –
Tadross 2014 2.22 0.95 – 2240 – – – –
Bukowiecki et al. 2011 2.81(1) 1.55 – 2239 – – – –
Dias et al. 2002 2.22 0.95 – 2239 – – – –

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

Visualization

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