HSC 1099

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0.56 UTI
0.55
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.8 [arcmin]
  • CN 0.55 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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HSC 1099 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Distant High extinction Massive Near-solar metallicity Intermediate age

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 – 37.119 60.148 0.267 -1.243 -0.812 -49.381
Hu & Soubiran 2025 37.123 60.143 – – – –
Hunt & Reffert 2024 37.12 60.137 0.271 -1.253 -0.794 -32.535
Cavallo et al. 2024 37.123 60.143 0.268 – – –
Hunt & Reffert 2023 37.12 60.137 0.271 -1.253 -0.794 -32.535

💡 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
Hu & Soubiran 2025 – – – – 0.040* – – –
Hunt & Reffert 2024 – – – – – 1159* – –
Cavallo et al. 2024 3.21 3.67 – 537 0.010 – – –
Hunt & Reffert 2023 3.24 3.77 1.67 205 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4038 100.0 37.13 60.15 0.27 -1.25 -0.81 -49.38 0.23

💡 Note: The % column shows the percentage of members that HSC 1099 shares with each listed object.

Visualization

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