HSC 538

Click to load Aladin Lite
0.40 UTI
0.26
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 0.8 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 538 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a large* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~5.85 kpc) differs significantly from the median photometric distance (~4.48 kpc).

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 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 – 299.841 30.063 0.171 -3.337 -6.03 –
Hunt & Reffert 2024 299.842 30.063 0.177 -3.341 -6.034 –
Cavallo et al. 2024 299.818 30.068 0.179 – – –
Hunt & Reffert 2023 299.842 30.063 0.177 -3.341 -6.034 –

💡 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 – – – – – 707* – –
Cavallo et al. 2024 3.58 2.77 – 60 0.180 – – –
Hunt & Reffert 2023 5.38 3.21 2.78 14 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3680 96.2 299.84 30.06 0.17 -3.34 -6.03 – 0.06

💡 Note: The % column shows the percentage of members that HSC 538 shares with each listed object.

Visualization

â„šī¸