HSC 2027

Click to load Aladin Lite
0.26 UTI
0.0
CN
0.29
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.29 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2027 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by low 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 Low 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 – 127.451 -32.265 0.172 -2.135 2.547 96.751
Hu & Soubiran 2025 127.438 -32.264 – – – –
Hunt & Reffert 2024 127.454 -32.263 0.162 -2.136 2.584 101.49
Cavallo et al. 2024 127.438 -32.264 0.16 – – –
Hunt & Reffert 2023 127.454 -32.263 0.162 -2.136 2.584 101.49

💡 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
Hu & Soubiran 2025 – – – – -0.180* – – –
Hunt & Reffert 2024 – – – – – 462* – –
Cavallo et al. 2024 3.75 0.73 – 603 -0.210 – – –
Hunt & Reffert 2023 5.32 0.68 2.03 557 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4758 96.0 127.45 -32.26 0.17 -2.14 2.54 90.11 0.03

💡 Note: The % column shows the percentage of members that HSC 2027 shares with each listed object.

Visualization

â„šī¸