NGC 7037

(MWSC 3477)

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0.20 UTI
0.0
CN
0.05
Cdens
0.38
CC3
0.29
Clit
1.0
Cdup
Core radius and density 2.9 [pc], 0.3 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.05 Very loose
  • CC3 0.38 Low quality
  • Clit 0.29 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
NGC 7037 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* 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 (~4.90 kpc) differs significantly from the median photometric distance (~2.47 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– 317.744 33.769 0.204 -3.672 -4.643 -74.855
Just et al. 2023 317.724 33.728 – – – –
Bica et al. 2019 317.706 33.747 – – – –
Dias et al. 2018 – – – -3.09 -5.34 –
Loktin & Popova 2017 317.73 33.763 – -0.212 -0.583 –
Sampedro et al. 2017 317.725 33.763 – 0.41 -3.53 –
Kharchenko et al. 2016 317.724 33.728 – – – –
Tadross 2014 317.725 33.763 – – – –
Dias et al. 2014 317.725 33.763 – 0.77 -3.53 –
Kharchenko et al. 2013 317.73 33.732 – -2.72 -1.0 –
Bukowiecki et al. 2011 317.783 33.771 – – – –
Dias et al. 2002 317.725 33.763 – 0.77 -3.53 –

💡 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– 2.47 1.985 – 501 – 977 – –
Just et al. 2023 – – – 37 – 977 – –
Loktin & Popova 2017 3.51 0.48 – 1622 – – – –
Kharchenko et al. 2016 2.47 5.26 – 37 – – – –
Tadross 2014 1.49 0.50 – 2100 – – – –
Kharchenko et al. 2013 2.47 5.26 – 37 – – – –
Bukowiecki et al. 2011 2.59(1) 0.06 – 3981 – – – –
Dias et al. 2002 1.76 3.47 – 501 – – – –

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

Visualization

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