NGC 6775

(MWSC 3079)

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0.17 UTI
0.0
CN
0.0
Cdens
0.25
CC3
0.29
Clit
1.0
Cdup
Core radius and density 5.5 [pc], 0.02 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.0 Very loose
  • CC3 0.25 Low quality
  • Clit 0.29 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
NGC 6775 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~6.31 kpc) differs significantly from the median photometric distance (~2.00 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.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 289.261 -0.958 0.159 -2.863 -5.667 60.877
Just et al. 2023 289.193 -0.924 – – – –
Bica et al. 2019 289.221 -0.92 – – – –
Dias et al. 2018 – – – -1.05 -3.1 –
Loktin & Popova 2017 289.245 -0.922 – 2.521 -8.672 –
Sampedro et al. 2017 289.2 -0.923 – – – –
Kharchenko et al. 2016 289.193 -0.924 – – – –
Tadross 2014 289.2 -0.923 – – – –
Dias et al. 2014 289.2 -0.923 – 0.19 -3.6 –
Kharchenko et al. 2013 289.2 -0.922 – 2.28 -7.45 –
Bukowiecki et al. 2011 289.192 0.941 – – – –
Dias et al. 2002 289.2 -0.923 – 2.28 -7.45 –

💡 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– 2.0 1.38 – 800 – 245 – –
Just et al. 2023 – – – 708 – 245 – –
Loktin & Popova 2017 2.63 0.81 – 1549 – – – –
Kharchenko et al. 2016 2.00 1.38 – 708 – – – –
Tadross 2014 1.19 1.51 – 900 – – – –
Kharchenko et al. 2013 2.00 1.38 – 708 – – – –
Dias et al. 2002 1.19 1.51 – 891 – – – –

Visualization

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