HSC 1106

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0.30 UTI
0.43
CN
0.68
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.6 [arcmin]
  • CN 0.43 Poorly populated
  • Cdens 0.68 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1106 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 38.994 60.31 0.457 0.128 -0.774 –
Hunt & Reffert 2024 39.047 60.309 0.455 0.144 -0.777 –
Cavallo et al. 2024 39.029 60.314 0.453 – – –
Hunt & Reffert 2023 39.047 60.309 0.455 0.144 -0.777 –

💡 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 – – – – – 355* – –
Cavallo et al. 2024 2.34 2.94 – 8 0.300 – – –
Hunt & Reffert 2023 2.11 2.90 1.94 14 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3324 74.4 39.02 60.31 0.46 0.12 -0.77 – 0.01

💡 Note: The % column shows the percentage of members that HSC 1106 shares with each listed object.

Visualization

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