HSC 129

Click to load Aladin Lite
0.39 UTI
0.31
CN
1.0
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.1 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 129 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above 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.
Relatively close High extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 270.694 -19.766 0.364 0.694 -1.464 24.057
Hunt & Reffert 2024 270.683 -19.761 0.355 0.712 -1.418 24.058
Cavallo et al. 2024 270.676 -19.765 0.357 – – –
Hunt & Reffert 2023 270.683 -19.761 0.355 0.712 -1.418 24.058

💡 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
Hunt & Reffert 2024 – – – – – 1111* – –
Cavallo et al. 2024 2.56 4.78 – 98 0.080 – – –
Hunt & Reffert 2023 2.51 4.83 2.65 106 – – – –

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

Visualization

â„šī¸