OC 0549

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0.37 UTI
0.28
CN
0.3
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 8.7 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.3 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0549 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Relatively close Low extinction Near-solar metallicity 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 – 158.315 -62.013 0.581 -5.605 5.337 60.53
Hunt & Reffert 2024 158.263 -62.006 0.572 -5.631 5.314 6.544
Cavallo et al. 2024 158.33 -62.019 0.573 – – –
Hunt & Reffert 2023 158.263 -62.006 0.572 -5.631 5.314 6.544
Hao et al. 2022 158.302 -62.031 0.584 -5.657 5.364 –

💡 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 – – – – – 192* – –
Cavallo et al. 2024 1.54 0.76 – 51 0.000 – – –
Hunt & Reffert 2023 1.65 0.57 0.36 118 – – – –
Hao et al. 2022 – 3.96 – 50 0.323 – – –

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

Visualization

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