OCSN 100

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0.65 UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 56.2 [arcmin]
  • CN 0.77 Rich
  • 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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OCSN 100 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, above 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 small percentage of members with at least one entry reported in the same catalogue. 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 – 242.706 -19.441 7.174 -8.761 -24.38 -7.18
Hunt & Reffert 2024 242.721 -19.383 7.193 -8.641 -24.329 -11.056
Cavallo et al. 2024 242.676 -19.339 7.195 – – –
Hunt & Reffert 2023 242.721 -19.383 7.193 -8.641 -24.329 -11.056
Qin et al. 2023 242.88 -19.41 7.19 -8.66 -24.36 -7.64

💡 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 – – – – – 59* – –
Cavallo et al. 2024 0.13 1.27 – 2 -0.290 – – –
Hunt & Reffert 2023 0.13 0.41 0.92 4 – – – –
Qin et al. 2023 0.19 0.90 – 7 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 96 11.2 240.86 -22.58 7.02 -11.74 -23.9 -7.43 0.67

💡 Note: The % column shows the percentage of members that OCSN 100 shares with each listed object.

Visualization

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