NGC 1663

(MWSC 426)

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0.23 UTI
0.0
CN
0.01
Cdens
0.38
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members) 7.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.01 Very loose
  • CC3 0.38 Low quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

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NGC 1663 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 old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~7.65 kpc) differs significantly from the median photometric distance (~1.49 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.

Relatively close Moderate extinction Old

Cantat-Gaudin et al. (2020)
Historically described as poor and irregular. Gaia DR2 data show large dispersion in proper motion and parallax, inconsistent with a physical cluster. More details in Appendix A of the article.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 72.344 13.114 0.131 0.516 -0.786 23.774
Just et al. 2023 72.307 13.169 – – – –
Angelo et al. 2019 72.35 13.14 – – – –
Loktin & Popova 2017 72.315 13.148 – 1.462 -7.315 –
Kharchenko et al. 2016 72.307 13.169 – – – –
Dias et al. 2014 72.242 13.148 – 2.18 -2.9 –
Kharchenko et al. 2013 72.315 13.17 – 2.56 -5.07 –

💡 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] Bfr BSS
Just et al. 2023 – – – 2512 – 309 – –
Angelo et al. 2019 2.40 – – 5010 – 15 – –
Loktin & Popova 2017 1.16 1.41 – 631 – – – –
Kharchenko et al. 2016 1.49 1.29 – 2512 – – – –
Kharchenko et al. 2013 1.49 1.29 – 2512 – – – –

Visualization

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