HSC 1259

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0.15 UTI
0.25
CN
0.14
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.5 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.14 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1259 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a large* distance, well above the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, intermediate-age cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~5.98 kpc) differs significantly from the median photometric distance (~4.17 kpc).

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Distant Moderate extinction Metal-poor 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 – 78.819 49.663 0.167 0.725 -0.486 -32.371
Hunt & Reffert 2024 78.81 49.664 0.167 0.678 -0.494 -0.518
Cavallo et al. 2024 78.796 49.707 0.169 – – –
Hunt & Reffert 2023 78.81 49.664 0.167 0.678 -0.494 -0.518

💡 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 – – – – – 180* – –
Cavallo et al. 2024 3.40 1.23 – 468 -0.650 – – –
Hunt & Reffert 2023 4.93 0.94 2.29 413 – – – –

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

Visualization

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