HSC 973

Click to load Aladin Lite
0.28 UTI
0.31
CN
0.35
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 6.4 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 0.35 Loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 973 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
Relatively close Low extinction Near-solar metallicity Young

Cavallo et al. (2024)
Bronze sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 11.115 55.263 0.442 -3.468 -1.825 -43.181
Zhang et al. 2024 11.105 55.204 – – – –
Hunt & Reffert 2024 11.105 55.204 0.442 -3.417 -1.828 –
Cavallo et al. 2024 11.127 55.437 0.447 – – –
Hunt & Reffert 2023 11.105 55.204 0.442 -3.417 -1.828 –

💡 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
Zhang et al. 2024 – – – – -0.323* – – –
Hunt & Reffert 2024 – – – – – 71* – –
Cavallo et al. 2024 2.91 1.10 – 19 0.140 – – –
Hunt & Reffert 2023 2.08 0.86 1.97 28 – – – –

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

Visualization

â„šī¸