HSC 549

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0.26 UTI
0.0
CN
0.29
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.29 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 549 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high 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.
Distant High 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 – 300.59 31.591 0.222 -2.389 -5.455 5.585
Hu & Soubiran 2025 300.583 31.605 – – – –
Hunt & Reffert 2024 300.578 31.597 0.229 -2.382 -5.444 13.226
Cavallo et al. 2024 300.583 31.605 0.226 – – –
Hunt & Reffert 2023 300.578 31.597 0.229 -2.382 -5.444 13.226

💡 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
Hu & Soubiran 2025 – – – – -0.040* – – –
Hunt & Reffert 2024 – – – – – 454* – –
Cavallo et al. 2024 4.74 3.07 – 501 -0.800 – – –
Hunt & Reffert 2023 4.00 3.01 1.94 466 – – – –

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

Visualization

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