HSC 508

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0.03 UTI
0.0
CN
0.08
Cdens
0.38
CC3
0.0
Clit
0.36
Cdup
Radius (P>50% members) 183.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.08 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.36 Possibly duplicate

Overview

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HSC 508 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very close distance, below 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.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Very close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 338.441 -0.816 7.087 22.409 -11.147 11.693
Zhang et al. 2024 338.43 -3.314 – – – –
Cavallo et al. 2024 338.845 -2.616 7.193 – – –
Hunt & Reffert 2023 338.43 -3.314 7.193 22.994 -10.635 9.568

💡 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 – – – – -0.024* – – –
Cavallo et al. 2024 0.14 0.48 – 93 0.060 – – –
Hunt & Reffert 2023 0.14 0.04 0.31 155 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1164 64.0 338.34 -0.35 6.78 21.13 -10.46 11.29 0.1

💡 Note: The % column shows the percentage of members that HSC 508 shares with each listed object.

Visualization

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