HSC 2309

Click to load Aladin Lite
0.07 UTI
0.0
CN
0.21
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 8.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.21 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2309 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a very small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

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.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 153.907 -56.27 0.556 -8.636 4.192 -2.86
Hunt & Reffert 2024 153.888 -56.26 0.564 -8.631 4.21 -2.915
Cavallo et al. 2024 154.008 -56.298 0.56 – – –
Hunt & Reffert 2023 153.888 -56.26 0.564 -8.631 4.21 -2.915

💡 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 – – – – – 102* – –
Cavallo et al. 2024 1.72 2.69 – 135 -0.020 – – –
Hunt & Reffert 2023 1.69 2.07 2.10 220 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 2306 8.0 153.72 -56.18 0.38 -8.72 4.26 18.73 0.17

💡 Note: The % column shows the percentage of members that HSC 2309 shares with each listed object.

Visualization

â„šī¸