HSC 1551

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0.10 UTI
0.0
CN
0.22
Cdens
0.62
CC3
0.0
Clit
0.6
Cdup
Radius (P>50% members) 15.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.22 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.6 Likely unique

Overview

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HSC 1551 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Close Low extinction Near-solar metallicity Very 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 – 92.852 13.986 1.055 -1.752 -1.375 19.186
Zhang et al. 2024 92.996 14.073 – – – –
Cavallo et al. 2024 92.735 13.763 1.044 – – –
Hunt & Reffert 2023 92.996 14.073 1.045 -1.767 -1.384 19.348

💡 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 – – – – -0.157* – – –
Cavallo et al. 2024 1.05 0.93 – 8 -0.050 – – –
Hunt & Reffert 2023 0.91 0.76 1.00 9 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 0946 40.0 92.75 14.12 1.03 -1.97 -1.42 11.21 0.44

💡 Note: The % column shows the percentage of members that HSC 1551 shares with each listed object.

Visualization

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