NGC 7084

(MWSC 3524)

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0.22 UTI
0.26
CN
0.1
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 8.2 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.1 Very loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
NGC 7084 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, well below the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~3.06 kpc) differs significantly from the median photometric distance (~1.59 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 Low extinction Old

Cantat-Gaudin et al. (2020)
Marked non-existent. Proper-motion analysis confirms lack of 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 – 323.041 17.58 0.327 -5.887 -7.365 6.133
Bica et al. 2019 322.952 17.418 – – – –
Loktin & Popova 2017 323.055 17.572 – -2.76 -10.027 –
Dias et al. 2014 323.137 17.508 – -1.39 -6.76 –
Dias et al. 2002 323.137 17.508 – -1.39 -6.76 –

💡 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
Loktin & Popova 2017 2.41 0.70 – 708 – – – –
Dias et al. 2002 0.77 0.31 – 1514 – – – –

Visualization

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