OC 0692

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0.02 UTI
0.64
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.03
Cdup
Radius (P>50% members) 2.7 [arcmin]
  • CN 0.64 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.03 Very likely duplicate

Overview

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OC 0692 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, 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.

(*): The parallax distance estimate (~3.60 kpc) differs significantly from the median photometric distance (~2.47 kpc).

Relatively close High extinction Massive Near-solar metallicity Very young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 263.377 -34.451 0.278 -0.72 -1.562 -12.781
Hunt & Reffert 2024 263.403 -34.442 0.285 -0.714 -1.549 -25.977
Cavallo et al. 2024 263.382 -34.444 0.285 – – –
Hunt & Reffert 2023 263.403 -34.442 0.285 -0.714 -1.549 -25.977
Hao et al. 2022 263.355 -34.489 0.282 -0.731 -1.659 -16.171

💡 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 – – – – – 3386* – –
Cavallo et al. 2024 1.79 5.17 – 12 -1.400 – – –
Hunt & Reffert 2023 3.15 4.54 1.58 19 – – – –
Hao et al. 2022 – 4.85 – 1 0.575 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 1199 97.4 263.4 -34.45 0.28 -0.68 -1.53 -12.34 0.55

💡 Note: The % column shows the percentage of members that OC 0692 shares with each listed object.

Visualization

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