HSC 1742

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0.36 UTI
0.29
CN
0.65
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 6.2 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 0.65 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1742 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
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 – 112.452 -4.117 0.604 -0.707 -0.403 15.798
Zhang et al. 2024 112.366 -4.125 – – – –
Hunt & Reffert 2024 112.366 -4.125 0.598 -0.713 -0.411 15.813
Cavallo et al. 2024 112.435 -4.136 0.605 – – –
Hunt & Reffert 2023 112.366 -4.125 0.598 -0.713 -0.411 15.813

💡 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 – – – – -0.208* – – –
Hunt & Reffert 2024 – – – – – 135* – –
Cavallo et al. 2024 1.44 0.17 – 282 0.130 – – –
Hunt & Reffert 2023 1.62 0.18 0.43 70 – – – –

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

Visualization

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