NGC 7036

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0.18 UTI
0.0
CN
0.06
Cdens
0.12
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad) 0.3 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.06 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.35 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
NGC 7036 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large* distance, well below the mid-plane, affected by low extinction. It is catalogued as a low-mass, old cluster (see Parameters). It is poorly studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~5.03 kpc) differs significantly from the median photometric distance (~1.08 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.

Cantat-Gaudin & Anders (2020)
Flagged as non-existent; Gaia DR2 data show no coherent kinematic group despite proposed members. 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 99999– 317.495 15.519 0.199 -3.334 -5.641 -33.245
Angelo et al. 2019 317.492 15.514 – – – –
Loktin & Popova 2017 317.505 15.517 – 1.44 -5.68 –
Bukowiecki et al. 2011 317.492 15.527 – – – –
van den Bergh 2006 317.508 15.518 – – – –
Dias et al. 2002 317.508 15.517 – 1.44 -5.68 –

💡 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– 1.08 0.185 – 3162 – 22 – –
Angelo et al. 2019 1.46 – – 2240 – 15 – –
Loktin & Popova 2017 1.38 0.06 – 2163 – – – –
Bukowiecki et al. 2012 – – – – – 28 – –
Bukowiecki et al. 2011 1.08(1) 0.00 – 3981 – – – –
van den Bergh 2006 1.00 0.31 – 3162 – – – –
Dias et al. 2002 1.00 0.31 – 3162 – – – –

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

Visualization

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