OMC 2

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0.17 UTI
0.0
CN
1.0
Cdens
0.25
CC3
0.0
Clit
0.68
Cdup
Stellar density (N50/rad) 104.4 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.68 Likely unique

Overview

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OMC 2 is a sparse, very dense object of low C3 quality. Its parallax locates it at a very close distance, below the mid-plane. It is catalogued as a cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 23 years.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Lada & Lada (2003)
Embedded cluster within âˆŧ2 Kpc of the Sun.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 83.855 -5.173 2.541 1.044 -0.025 26.687
Lada & Lada 2003 83.864 -5.161 – – – –

💡 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] Bfrac BSS
UCC 99999– 0.5 – – – – 63 – –
Lada & Lada 2003 0.50 – – – – 63 – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 225 96.0 83.84 -4.96 2.55 1.25 -0.08 22.73 0.36
NGC 1976 32.0 83.82 -5.45 2.58 1.25 0.19 19.86 0.78
NGC 1977 20.0 83.84 -4.86 2.53 1.26 -0.71 23.87 0.82
UBC 621 20.0 83.83 -4.86 2.53 1.25 -0.72 22.95 0.05
OC 0345 12.0 83.77 -5.87 2.58 1.06 0.21 19.86 0.03
OCSN 244 8.0 83.82 -5.43 2.52 1.39 0.33 25.62 0.25

💡 Note: The % column shows the percentage of members that OMC 2 shares with each listed object.

Visualization

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