HSC 258

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0.02 UTI
0.44
CN
0.76
Cdens
0.75
CC3
0.0
Clit
0.04
Cdup
Radius (P>50% members) 4.7 [arcmin]
  • CN 0.44 Poorly populated
  • Cdens 0.76 Dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.04 Very likely duplicate

Overview

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HSC 258 is a poorly populated, dense object of high 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, young cluster (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 High extinction Near-solar metallicity 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 – 278.423 -4.931 0.402 -0.558 -2.383 –
Hunt & Reffert 2024 278.423 -4.874 0.411 -0.565 -2.371 –
Cavallo et al. 2024 278.422 -4.954 0.404 – – –
Hunt & Reffert 2023 278.423 -4.874 0.411 -0.565 -2.371 –

💡 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 – – – – – 634* – –
Cavallo et al. 2024 3.05 3.27 – 32 0.360 – – –
Hunt & Reffert 2023 2.33 3.26 2.26 23 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
IRAS 18306-0500 95.5 278.4 -4.97 0.4 -0.56 -2.38 -3.16 0.45

💡 Note: The % column shows the percentage of members that HSC 258 shares with each listed object.

Visualization

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