MVM2011 G37.51-0.46

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0.13 UTI
0.27
CN
0.27
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 1.3 [N/pc2]
  • CN 0.27 Poorly populated
  • Cdens 0.27 Loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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MVM2011 G37.51-0.46 is a poorly populated, loose object of very low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane. It is catalogued as a cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 13 years.

(*): The parallax distance estimate (~3.03 kpc) differs significantly from the median photometric distance (~6.10 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.

Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 285.413 3.841 0.33 -2.05 -4.932 43.498
Morales et al. 2013 285.363 3.867 – – – –

💡 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– 6.1 – – – – – – –
Morales et al. 2013 6.10 – – – – – – –

Visualization

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