HSC 285

Click to load Aladin Lite
0.49 UTI
0.45
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.9 [arcmin]
  • CN 0.45 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 285 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a metal-poor, young 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 Very high extinction Metal-poor 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 – 280.905 -3.816 0.307 -0.726 -1.88 44.129
Hunt & Reffert 2024 280.907 -3.814 0.302 -0.733 -1.899 70.223
Cavallo et al. 2024 280.902 -3.815 0.301 – – –
Hunt & Reffert 2023 280.907 -3.814 0.302 -0.733 -1.899 70.223

💡 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 – – – – – 964* – –
Cavallo et al. 2024 2.74 5.20 – 46 -0.580 – – –
Hunt & Reffert 2023 2.96 5.03 2.31 50 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3278 100.0 280.9 -3.82 0.31 -0.72 -1.88 44.13 0.17

💡 Note: The % column shows the percentage of members that HSC 285 shares with each listed object.

Visualization

â„šī¸