HSC 305

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0.03 UTI
0.25
CN
0.38
Cdens
0.38
CC3
0.0
Clit
0.16
Cdup
Radius (P>50% members) 29.6 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.38 Loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.16 Likely duplicate

Overview

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HSC 305 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low 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 likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Very close Low extinction Near-solar metallicity Young

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 – 269.764 2.931 2.378 0.054 -8.208 -13.406
Zhang et al. 2024 269.716 4.105 – – – –
Cavallo et al. 2024 269.721 3.307 2.395 – – –
Hunt & Reffert 2023 269.716 4.105 2.402 -0.01 -8.381 -26.559

💡 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 – – – – -0.060* – – –
Cavallo et al. 2024 0.44 0.69 – 7 -0.330 – – –
Hunt & Reffert 2023 0.41 0.45 0.71 175 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1188 84.0 269.91 2.93 2.36 0.14 -8.26 -14.99 0.25

💡 Note: The % column shows the percentage of members that HSC 305 shares with each listed object.

Visualization

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