HSC 198

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0.42 UTI
0.37
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 1.3 [arcmin]
  • CN 0.37 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 198 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Distant Very high extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 276.095 -14.49 0.272 -1.771 -4.628 4.92
Hunt & Reffert 2024 276.1 -14.49 0.283 -1.745 -4.621 27.384
Cavallo et al. 2024 276.099 -14.489 0.283 – – –
Hunt & Reffert 2023 276.1 -14.49 0.283 -1.745 -4.621 27.384

💡 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
Hunt & Reffert 2024 – – – – – 1456* – –
Cavallo et al. 2024 3.12 4.91 – 204 -0.300 – – –
Hunt & Reffert 2023 3.28 5.33 2.85 226 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3172 100.0 276.1 -14.49 0.27 -1.74 -4.62 5.0 0.33

💡 Note: The % column shows the percentage of members that HSC 198 shares with each listed object.

Visualization

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