PHOC 17

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0.49 UTI
0.75
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.75
Cdup
Stellar density (N50/rad) 20.0 [N/pc2]
  • CN 0.75 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.75 Very likely unique

Overview

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PHOC 17 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, metal-rich, very young cluster (see Parameters). It is poorly studied in the literature.

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

Palma et al. (2025)
Part of multiple system G173, along with UFMG_66 and HSC_2929.

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– 261.171 -34.685 0.599 -1.277 -3.123 -1.583
Hunt & Reffert 2024 261.175 -34.705 0.592 -1.251 -3.125 28.132
Cavallo et al. 2024 261.169 -34.687 0.592 – – –
Hunt & Reffert 2023 261.175 -34.705 0.592 -1.251 -3.125 28.132
Hunt & Reffert 2021 261.174 -34.687 0.558 -1.265 -3.105 –

💡 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– 1.66 5.175 1.95 12 0.870 1309 – –
Hunt & Reffert 2024 – – – – – 1309(1) – –
Cavallo et al. 2024 1.70 4.97 – 17 0.870 – – –
Hunt & Reffert 2023 1.62 5.38 1.95 6 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UFMG 76 63.3 261.17 -34.69 0.59 -1.24 -3.13 -1.58 0.0
CWWDL 13876 45.0 261.16 -34.69 0.6 -1.26 -3.15 -1.58 0.0
G3CC 47 24.8 260.85 -34.8 0.6 -0.86 -3.02 -14.93 0.44

💡 Note: The % column shows the percentage of members that PHOC 17 shares with each listed object.

Visualization

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