HSC 919

Click to load Aladin Lite
0.45 UTI
0.25
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 0.6 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 919 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate 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 large percentage of members with a later reported entry. See table with shared members information.

Distant Moderate 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 – 356.521 62.278 0.214 -2.091 -0.699 –
Hunt & Reffert 2024 356.516 62.276 0.212 -2.136 -0.708 -78.416
Cavallo et al. 2024 356.513 62.293 0.21 – – –
Hunt & Reffert 2023 356.516 62.276 0.212 -2.136 -0.708 -78.416

💡 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 – – – – – 446* – –
Cavallo et al. 2024 3.42 2.72 – 148 -0.430 – – –
Hunt & Reffert 2023 4.25 2.90 1.65 170 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3748 100.0 356.53 62.28 0.2 -2.07 -0.7 -65.22 0.22

💡 Note: The % column shows the percentage of members that HSC 919 shares with each listed object.

Visualization

â„šī¸