HSC 1314

Click to load Aladin Lite
0.03 UTI
0.0
CN
0.21
Cdens
0.25
CC3
0.0
Clit
0.32
Cdup
Radius (P>50% members) 46.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.21 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.32 Possibly duplicate

Overview

â„šī¸
HSC 1314 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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 Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

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

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 72.765 36.672 2.894 3.29 -10.77 4.917
Zhang et al. 2024 74.422 35.931 – – – –
Cavallo et al. 2024 71.903 37.348 2.851 – – –
Hunt & Reffert 2023 74.422 35.931 2.855 3.396 -10.641 4.192

💡 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 – – – – 0.279* – – –
Cavallo et al. 2024 0.36 1.22 – 135 0.600 – – –
Hunt & Reffert 2023 0.34 1.18 1.46 117 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 1362 68.0 73.33 36.54 2.91 3.24 -10.78 6.39 0.15

💡 Note: The % column shows the percentage of members that HSC 1314 shares with each listed object.

Visualization

â„šī¸