HSC 749

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0.06 UTI
0.25
CN
0.09
Cdens
0.25
CC3
0.0
Clit
0.52
Cdup
Radius (P>50% members) 209.5 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.09 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.52 Likely unique

Overview

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HSC 749 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a very 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 likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Very close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 6.058 2.707 8.226 18.258 -14.783 12.493
Zhang et al. 2024 358.47 3.455 – – – –
Cavallo et al. 2024 5.95 2.012 8.109 – – –
Hunt & Reffert 2023 358.47 3.455 8.128 18.061 -13.839 16.442

💡 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 – – – – 0.034* – – –
Cavallo et al. 2024 0.13 0.50 – 309 0.170 – – –
Hunt & Reffert 2023 0.12 0.07 0.45 226 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1077 48.0 9.5 1.9 8.43 17.55 -14.39 15.68 0.17

💡 Note: The % column shows the percentage of members that HSC 749 shares with each listed object.

Visualization

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