OC 0377

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0.00 UTI
0.28
CN
1.0
Cdens
0.62
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members) 4.8 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
OC 0377 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young 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.

Relatively close Low extinction Near-solar metallicity Very young

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 – 107.417 -12.038 0.853 -3.258 0.937 20.73
Hunt & Reffert 2024 107.413 -12.049 0.85 -3.174 0.88 26.879
Cavallo et al. 2024 107.418 -12.301 0.85 – – –
Hunt & Reffert 2023 107.413 -12.049 0.85 -3.174 0.88 26.879
Hao et al. 2022 107.396 -12.044 0.856 -3.277 0.926 –

💡 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 – – – – – 267* – –
Cavallo et al. 2024 1.12 0.79 – 12 0.060 – – –
Hunt & Reffert 2023 1.10 0.79 1.46 14 – – – –
Hao et al. 2022 – 2.02 – 8 0.611 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CMa08 100.0 107.43 -12.28 0.86 -3.15 0.88 26.44 0.5
CWWDL 14343 78.6 107.36 -12.04 0.85 -3.28 0.96 21.1 0.01
CWWDL 14345 78.6 107.43 -12.14 0.87 -3.2 0.92 22.81 0.01

💡 Note: The % column shows the percentage of members that OC 0377 shares with each listed object.

Visualization

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