HSC 1041

Click to load Aladin Lite
0.31 UTI
0.0
CN
0.56
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.56 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1041 is a sparse, moderately dense object of intermediate 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 – 28.156 65.386 0.25 -0.07 0.348 -50.931
Hu & Soubiran 2025 28.111 65.386 – – – –
Hunt & Reffert 2024 28.171 65.386 0.251 -0.082 0.367 -50.658
Cavallo et al. 2024 28.111 65.386 0.252 – – –
Hunt & Reffert 2023 28.171 65.386 0.251 -0.082 0.367 -50.658

💡 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 – – – – 0.010* – – –
Hunt & Reffert 2024 – – – – – 418* – –
Cavallo et al. 2024 3.91 2.60 – 525 0.000 – – –
Hunt & Reffert 2023 3.67 2.43 1.36 546 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3034 96.0 28.16 65.38 0.25 -0.09 0.35 -50.93 0.18

💡 Note: The % column shows the percentage of members that HSC 1041 shares with each listed object.

Visualization

â„šī¸