OC 0370

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0.00 UTI
0.74
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members) 11.5 [arcmin]
  • CN 0.74 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
OC 0370 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 107.266 -7.186 1.136 -0.89 -1.19 1.12
Hunt & Reffert 2024 107.261 -7.202 1.141 -0.868 -1.133 1.611
Cavallo et al. 2024 107.234 -7.195 1.135 – – –
Hunt & Reffert 2023 107.261 -7.202 1.141 -0.868 -1.133 1.611
Hao et al. 2022 107.249 -7.168 1.146 -0.867 -1.099 14.553

💡 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
Hunt & Reffert 2024 – – – – – 339* – –
Cavallo et al. 2024 0.87 0.25 – 178 0.140 – – –
Hunt & Reffert 2023 0.83 0.19 0.72 159 – – – –
Hao et al. 2022 – 0.26 – 79 0.611 – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FOF 2302 100.0 107.26 -7.2 1.14 -0.9 -1.2 3.48 0.5
CWWDL 14377 95.9 107.26 -7.19 1.14 -0.89 -1.2 1.22 0.01
Theia 361 20.6 107.27 -7.22 1.17 -0.92 -1.16 6.2 0.01

💡 Note: The % column shows the percentage of members that OC 0370 shares with each listed object.

Visualization

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