HSC 1193

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0.02 UTI
0.0
CN
1.0
Cdens
0.38
CC3
0.25
Clit
0.04
Cdup
Radius (P>50% members) 4.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.04 Very likely duplicate

Overview

â„šī¸
HSC 1193 is a sparse, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate 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.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 59.913 51.601 0.929 -0.047 -1.981 3.014
Zhang et al. 2024 59.964 51.594 – – – –
Hunt & Reffert 2024 59.964 51.594 0.92 -0.022 -1.965 3.415
Cavallo et al. 2024 59.927 51.602 0.921 – – –
Hunt & Reffert 2023 59.964 51.594 0.92 -0.022 -1.965 3.415

💡 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 – – – – -0.215* – – –
Hunt & Reffert 2024 – – – – – 82* – –
Cavallo et al. 2024 1.10 1.39 – 13 0.560 – – –
Hunt & Reffert 2023 1.05 1.76 1.39 8 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1220 96.0 59.88 51.67 0.94 -0.05 -1.98 4.06 0.4

💡 Note: The % column shows the percentage of members that HSC 1193 shares with each listed object.

Visualization

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