OC 0497

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0.55 UTI
0.26
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.1 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0497 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 137.854 -45.584 1.321 -8.431 3.923 -1.189
Hunt & Reffert 2024 137.852 -45.568 1.291 -8.559 4.068 -2.182
Cavallo et al. 2024 137.885 -45.547 1.313 – – –
Hunt & Reffert 2023 137.852 -45.568 1.291 -8.559 4.068 -2.182
Hao et al. 2022 137.852 -45.573 1.328 -8.436 3.893 –

💡 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 – – – – – 89* – –
Cavallo et al. 2024 1.01 1.78 – 2 0.040 – – –
Hunt & Reffert 2023 0.73 1.53 2.06 4 – – – –
Hao et al. 2022 – 0.82 – 2 0.498 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 208 92.3 137.85 -45.58 1.33 -8.41 3.93 -1.19 0.02

💡 Note: The % column shows the percentage of members that OC 0497 shares with each listed object.

Visualization

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