HSC 1913

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0.00 UTI
0.27
CN
0.27
Cdens
0.75
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members) 18.1 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.27 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
HSC 1913 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a close distance, below 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.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large 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.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 106.331 -27.767 1.186 -3.133 3.385 32.811
Hunt & Reffert 2024 106.266 -27.796 1.188 -3.134 3.402 36.903
Cavallo et al. 2024 106.367 -27.813 1.192 – – –
Hunt & Reffert 2023 106.266 -27.796 1.188 -3.134 3.402 36.903

💡 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 – – – – – 92* – –
Cavallo et al. 2024 0.88 0.39 – 7 -0.120 – – –
Hunt & Reffert 2023 0.81 0.12 0.43 12 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14295 100.0 106.33 -27.81 1.19 -3.12 3.4 32.31 0.38
OC 0410 29.6 105.73 -27.38 1.2 -3.1 3.48 35.18 0.13

💡 Note: The % column shows the percentage of members that HSC 1913 shares with each listed object.

Visualization

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