HSC 264

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0.35 UTI
0.0
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.3 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 264 is a sparse, very dense object of 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 massive, 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.

Distant Very high extinction Massive Young

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 280.586 -5.785 0.201 -1.189 -2.848 50.595
Hunt & Reffert 2024 280.583 -5.784 0.194 -1.194 -2.805 50.345
Hunt & Reffert 2023 280.583 -5.784 0.194 -1.194 -2.805 50.345

💡 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 – – – – – 1290* – –
Hunt & Reffert 2023 4.25 5.76 1.77 31 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3646 92.0 280.59 -5.78 0.21 -1.18 -2.84 49.8 0.18

💡 Note: The % column shows the percentage of members that HSC 264 shares with each listed object.

Visualization

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