OCSN 27

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0.67 UTI
0.71
CN
1.0
Cdens
1.0
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 26.0 [arcmin]
  • CN 0.71 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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OCSN 27 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

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

Very 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 – 321.634 47.638 2.421 3.328 -2.486 -15.463
Zhang et al. 2024 321.607 47.633 – – – –
Hunt & Reffert 2024 321.607 47.633 2.407 3.257 -2.506 -16.306
Cavallo et al. 2024 320.857 47.609 2.402 – – –
Hunt & Reffert 2023 321.607 47.633 2.407 3.257 -2.506 -16.306
Qin et al. 2023 321.68 47.54 2.41 3.3 -2.53 -15.23

💡 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
Zhang et al. 2024 – – – – 0.089* – – –
Hunt & Reffert 2024 – – – – – 64* – –
Cavallo et al. 2024 0.43 0.56 – 10 -0.100 – – –
Hunt & Reffert 2023 0.41 0.15 0.49 15 – – – –
Qin et al. 2023 0.49 0.34 – 22 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14619 53.3 321.77 47.67 2.42 3.37 -2.49 -16.28 0.0

💡 Note: The % column shows the percentage of members that OCSN 27 shares with each listed object.

Visualization

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