HSC 1539

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0.26 UTI
0.34
CN
0.23
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 21.3 [arcmin]
  • CN 0.34 Poorly populated
  • Cdens 0.23 Very loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1539 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
Close Low extinction Near-solar metallicity Young

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 – 90.729 14.594 1.15 -1.599 -1.528 5.228
Zhang et al. 2024 90.691 14.594 – – – –
Hunt & Reffert 2024 90.691 14.594 1.145 -1.577 -1.491 14.879
Cavallo et al. 2024 90.674 14.596 1.145 – – –
Hunt & Reffert 2023 90.691 14.594 1.145 -1.577 -1.491 14.879

💡 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 – – – – -0.185* – – –
Hunt & Reffert 2024 – – – – – 95* – –
Cavallo et al. 2024 1.01 0.53 – 19 0.150 – – –
Hunt & Reffert 2023 0.83 0.37 0.86 36 – – – –

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

Visualization

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