HSC 210

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0.06 UTI
0.0
CN
0.76
Cdens
0.25
CC3
0.0
Clit
0.28
Cdup
Radius (P>50% members) 4.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.76 Dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.28 Possibly duplicate

Overview

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HSC 210 is a sparse, dense object of 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 young cluster (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.

Relatively close Moderate extinction Young

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 277.308 -12.7 0.572 0.547 -1.618 –
Hunt & Reffert 2024 277.341 -12.67 0.677 0.532 -1.603 –
Hunt & Reffert 2023 277.341 -12.67 0.677 0.532 -1.603 –

💡 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 – – – – – 88* – –
Hunt & Reffert 2023 1.42 2.23 1.26 37 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1020 72.0 277.26 -12.72 0.46 0.62 -1.65 10.83 0.66
CWNU 506 28.0 277.25 -12.72 0.48 0.64 -1.67 17.92 0.0
OC 0032 20.0 277.26 -12.73 0.48 0.62 -1.66 88.27 0.0
CWNU 44 16.0 277.26 -12.72 0.47 0.61 -1.66 18.06 0.0

💡 Note: The % column shows the percentage of members that HSC 210 shares with each listed object.

Visualization

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