PTB 9

(MWSC 3763)

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0.01 UTI
1.0
CN
1.0
Cdens
1.0
CC3
0.45
Clit
0.02
Cdup
Stellar density (N50/rad) 81.8 [N/pc2]
  • CN 1.0 Very rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.45 Poorly studied
  • Cdup 0.02 Very likely duplicate

Overview

â„šī¸
PTB 9 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the mass parameter (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.

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 99999– 357.454 68.038 1.032 1.484 3.979 -44.717
Hu & Soubiran 2025 357.449 68.04 – – – –
Hunt & Reffert 2024 357.495 68.031 1.033 1.482 3.963 -44.265
Cavallo et al. 2024 357.449 68.04 1.033 – – –
Hunt & Reffert 2023 357.495 68.031 1.033 1.482 3.963 -44.265
Just et al. 2023 357.495 68.03 – – – –
Kharchenko et al. 2016 357.495 68.03 – – – –
Kharchenko et al. 2013 357.502 68.033 – -2.8 0.04 –
Kharchenko et al. 2012 357.502 68.033 – -2.8 0.04 –

💡 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– 0.85 2.17 1.04 1175 0.060 1387 – –
Hu & Soubiran 2025 – – – – 0.150(5) – – –
Hunt & Reffert 2024 – – – – – 2676(1) – –
Cavallo et al. 2024 1.04 2.89 – 813 -0.030 – – –
Hunt & Reffert 2023 0.93 2.55 1.04 871 – – – –
Just et al. 2023 – – – 1175 – 98 – –
Kharchenko et al. 2016 0.85 2.17 – 1175 – – – –
Kharchenko et al. 2013 0.85 2.17 – 1175 – – – –
Kharchenko et al. 2012 0.85 2.17 – 1175 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Melotte 244 98.1 357.45 68.04 1.03 1.48 3.98 -44.73 1.0

💡 Note: The % column shows the percentage of members that PTB 9 shares with each listed object.

Visualization

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