HSC 1902

Click to load Aladin Lite
0.39 UTI
0.36
CN
0.96
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 12.4 [arcmin]
  • CN 0.36 Poorly populated
  • Cdens 0.96 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1902 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Close Low extinction Low mass Near-solar metallicity Young

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 – 109.803 -24.921 1.316 -3.159 4.822 40.16
Hunt & Reffert 2024 109.823 -24.978 1.315 -3.177 4.838 37.682
Cavallo et al. 2024 109.687 -24.553 1.321 – – –
Hunt & Reffert 2023 109.823 -24.978 1.315 -3.177 4.838 37.682

💡 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 – – – – – 44* – –
Cavallo et al. 2024 0.80 0.39 – 17 0.050 – – –
Hunt & Reffert 2023 0.73 0.20 0.71 31 – – – –

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

Visualization

â„šī¸