HSC 1284

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0.06 UTI
0.0
CN
0.32
Cdens
0.62
CC3
0.0
Clit
0.32
Cdup
Radius (P>50% members) 11.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.32 Loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.32 Possibly duplicate

Overview

HSC 1284 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. It is catalogued as a near-solar metallicity cluster (see Parameters). It was recently reported in the literature.

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.

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 72.955 40.795 0.896 1.706 -5.882 -6.54
Zhang et al. 2024 72.943 40.855
Hunt & Reffert 2024 72.943 40.855 0.87 1.635 -5.771 -2.508

💡 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 -0.214*
Hunt & Reffert 2024 87*

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
(*): indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4058 68.0 73.19 40.65 0.88 1.67 -5.87 -3.03 0.15

💡 Note: The % column shows the percentage of members that HSC 1284 shares with each listed object.

Visualization

Galactocentric position diagram

💡 Note: How are the galactocentric plots generated? See FAQ.