HSC 1523

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0.33 UTI
0.25
CN
0.66
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 34.1 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.66 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1523 is a poorly populated, moderately dense object of high 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, very young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
Very close Low extinction Near-solar metallicity Very young

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 – 79.151 9.933 3.593 1.539 -3.78 19.415
Zhang et al. 2024 79.014 10.036 – – – –
Cavallo et al. 2024 79.036 9.892 3.569 – – –
Hunt & Reffert 2023 79.014 10.036 3.585 1.52 -3.816 14.331

💡 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 – – – – 0.203* – – –
Cavallo et al. 2024 0.28 0.80 – 13 0.550 – – –
Hunt & Reffert 2023 0.27 0.25 0.41 13 – – – –

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

Visualization

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