HSC 1577

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0.28 UTI
0.0
CN
0.14
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.0 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.14 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1577 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Distant 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 – 99.296 14.248 0.27 -0.232 -1.097 65.245
Zhang et al. 2024 99.301 14.223 – – – –
Hunt & Reffert 2024 99.301 14.223 0.277 -0.227 -1.09 –
Cavallo et al. 2024 99.295 14.248 0.277 – – –
Hunt & Reffert 2023 99.301 14.223 0.277 -0.227 -1.09 –

💡 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 – – – – 0.224* – – –
Hunt & Reffert 2024 – – – – – 169* – –
Cavallo et al. 2024 3.55 0.90 – 347 0.310 – – –
Hunt & Reffert 2023 3.40 0.67 0.85 208 – – – –

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

Visualization

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