Gulliver 16

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0.46 UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.77
Cdup
Radius (P>50% members) 2.5 [arcmin]
  • CN 0.75 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.77 Very likely unique

Overview

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Gulliver 16 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature, with no articles listed in the last 6 years.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

Distant Moderate extinction Near-solar metallicity Young

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 23.423 60.749 0.215 -1.28 -0.654 -37.022
Cantat-Gaudin et al. 2020 23.433 60.751 0.208 -1.249 -0.614 –
Cantat-Gaudin & Anders 2020 23.433 60.751 0.208 -1.249 -0.614 –
Monteiro & Dias 2019 23.433 60.751 – – – 3.016
Cantat-Gaudin et al. 2018 23.433 60.751 0.208 -1.249 -0.614 –

💡 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
Cantat-Gaudin et al. 2020 4.90 1.39 – 141 – – – –
Cantat-Gaudin & Anders 2020 4.22 – – – – – – –
Monteiro & Dias 2019 8.76 1.81 – 7 0.050 – – –
Cantat-Gaudin et al. 2018 4.22 – – – – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Schoenball 1 97.0 23.42 60.75 0.23 -1.29 -0.65 -37.74 0.16
NGC 581 23.0 23.34 60.66 0.36 -1.4 -0.58 -38.14 0.96
CWWDL 6155 6.0 23.23 60.63 0.34 -1.26 -0.61 – 0.05
UBC 186 3.0 23.47 60.66 0.34 -1.34 -0.51 – 0.11
Teutsch J0135.2+6041 1.0 23.44 60.67 0.36 -1.44 -0.61 -38.14 0.09

💡 Note: The % column shows the percentage of members that Gulliver 16 shares with each listed object.

Visualization

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