HSC 734

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0.41 UTI
0.74
CN
0.35
Cdens
0.75
CC3
0.25
Clit
0.88
Cdup
Radius (P>50% members) 20.1 [arcmin]
  • CN 0.74 Moderately populated
  • Cdens 0.35 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.88 Very likely unique

Overview

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HSC 734 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, below 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 is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Low extinction Near-solar metallicity 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 – 327.659 45.503 0.791 2.275 -0.049 -13.66
Zhang et al. 2024 327.731 45.479 – – – –
Hunt & Reffert 2024 327.731 45.479 0.778 2.178 -0.058 -16.702
Cavallo et al. 2024 326.826 45.29 0.78 – – –
Hunt & Reffert 2023 327.731 45.479 0.778 2.178 -0.058 -16.702

💡 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
Zhang et al. 2024 – – – – 0.012* – – –
Hunt & Reffert 2024 – – – – – 164* – –
Cavallo et al. 2024 1.28 0.80 – 178 0.190 – – –
Hunt & Reffert 2023 1.23 0.53 0.72 245 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HXHWL 41 12.4 326.74 45.26 0.77 2.16 -0.03 -28.12 0.14

💡 Note: The % column shows the percentage of members that HSC 734 shares with each listed object.

Visualization

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