HSC 265

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0.30 UTI
0.3
CN
0.47
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.6 [arcmin]
  • CN 0.3 Poorly populated
  • Cdens 0.47 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 265 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-poor, 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.

Relatively close High extinction Metal-poor Intermediate age

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 – 279.862 -5.35 0.293 0.243 -2.201 131.378
Hunt & Reffert 2024 279.835 -5.379 0.303 0.237 -2.214 77.392
Cavallo et al. 2024 279.856 -5.36 0.304 – – –
Hunt & Reffert 2023 279.835 -5.379 0.303 0.237 -2.214 77.392

💡 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 – – – – – 712* – –
Cavallo et al. 2024 2.43 4.11 – 151 -0.560 – – –
Hunt & Reffert 2023 3.19 3.98 1.76 57 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3527 100.0 279.87 -5.35 0.29 0.24 -2.19 131.38 0.16

💡 Note: The % column shows the percentage of members that HSC 265 shares with each listed object.

Visualization

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