Sco OB5

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0.55 UTI
0.5
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 7.0 [N/pc2]
  • CN 0.5 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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Sco OB5 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close* distance, below the mid-plane, affected by low extinction. It is catalogued as an extremely massive, very young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~1.22 kpc) differs significantly from the median photometric distance (~3.31 kpc).

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 268.109 -38.704 0.817 2.902 -1.812 -14.824
He et al. 2023 268.137 -38.728 0.804 2.884 -1.796 -17.98
Piskunov et al. 2008 268.129 -38.644 – – – –
Piskunov et al. 2007 268.129 -38.644 – – – –
Kharchenko et al. 2005 268.14 -38.64 – 2.46 -1.8 –

💡 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– 3.31 0.71 – 7 – 349626 – –
He et al. 2023 1.29 1.00 – 16 – – – –
Piskunov et al. 2008 3.31 0.71 – 7 – 588844(1) – –
Piskunov et al. 2007 3.31 0.71 – 7 – 110408 – –
Kharchenko et al. 2005 3.31 0.71 – 7 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Alessi 80B 98.0 268.11 -38.69 0.81 2.9 -1.77 -17.98 0.21

💡 Note: The % column shows the percentage of members that Sco OB5 shares with each listed object.

Visualization

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