HSC 2919

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0.00 UTI
0.78
CN
1.0
Cdens
0.62
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members) 38.5 [arcmin]
  • CN 0.78 Rich
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
HSC 2919 is a rich, very dense object of intermediate C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, 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.

Very close High extinction Near-solar metallicity Young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 246.54 -24.018 7.209 -6.805 -25.977 -8.441
Hunt & Reffert 2024 246.602 -24.085 7.215 -6.932 -26.018 -19.331
Cavallo et al. 2024 246.483 -24.045 7.212 – – –
Hunt & Reffert 2023 246.602 -24.085 7.215 -6.932 -26.018 -19.331

💡 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 – – – – – 60* – –
Cavallo et al. 2024 0.15 4.02 – 14 0.220 – – –
Hunt & Reffert 2023 0.13 3.22 2.40 27 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 245 100.0 246.4 -24.04 7.2 -7.05 -25.65 -7.74 0.53
OC 0690 23.0 246.39 -23.48 7.18 -6.96 -25.51 -7.74 0.48

💡 Note: The % column shows the percentage of members that HSC 2919 shares with each listed object.

Visualization

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