HSC 35

Click to load Aladin Lite
0.57 UTI
0.35
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.5 [arcmin]
  • CN 0.35 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 35 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Relatively close High extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 266.965 -26.128 0.527 -0.527 -0.807 -17.887
Hu & Soubiran 2025 266.959 -26.132 – – – –
Hunt & Reffert 2024 266.987 -26.124 0.535 -0.533 -0.809 -6.423
Cavallo et al. 2024 266.959 -26.132 0.531 – – –
Hunt & Reffert 2023 266.987 -26.124 0.535 -0.533 -0.809 -6.423

💡 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 – – – – -0.110* – – –
Hunt & Reffert 2024 – – – – – 460* – –
Cavallo et al. 2024 1.20 3.40 – 501 -0.040 – – –
Hunt & Reffert 2023 1.76 3.36 2.34 78 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4314 71.4 266.97 -26.13 0.53 -0.53 -0.79 -12.65 0.0

💡 Note: The % column shows the percentage of members that HSC 35 shares with each listed object.

Visualization

â„šī¸