HSC 294

Click to load Aladin Lite
0.33 UTI
0.29
CN
1.0
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.7 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 294 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate 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 large 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 – 282.478 -3.506 0.494 0.82 -1.601 4.235
Hunt & Reffert 2024 282.488 -3.489 0.489 0.798 -1.588 4.235
Cavallo et al. 2024 282.483 -3.531 0.486 – – –
Hunt & Reffert 2023 282.488 -3.489 0.489 0.798 -1.588 4.235

💡 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 – – – – – 399* – –
Cavallo et al. 2024 1.84 3.56 – 240 0.470 – – –
Hunt & Reffert 2023 1.90 3.74 2.28 156 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3239 100.0 282.47 -3.51 0.49 0.82 -1.6 23.28 0.09

💡 Note: The % column shows the percentage of members that HSC 294 shares with each listed object.

Visualization

â„šī¸