HSC 1844

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0.09 UTI
0.0
CN
0.22
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 8.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.22 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1844 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a metal-rich, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. 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 Low extinction Metal-rich 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 – 110.261 -19.43 0.61 -3.092 1.948 53.233
Cavallo et al. 2024 110.286 -19.454 0.602 – – –
Hunt & Reffert 2023 110.277 -19.433 0.594 -3.1 1.907 58.154

💡 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
Cavallo et al. 2024 1.61 0.50 – 282 0.500 – – –
Hunt & Reffert 2023 1.57 0.29 0.18 255 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3770 84.0 110.24 -19.42 0.61 -3.07 1.96 53.23 0.02

💡 Note: The % column shows the percentage of members that HSC 1844 shares with each listed object.

Visualization

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