HSC 2910

Click to load Aladin Lite
0.11 UTI
0.41
CN
0.17
Cdens
0.38
CC3
0.0
Clit
0.58
Cdup
Radius (P>50% members) 17.3 [arcmin]
  • CN 0.41 Poorly populated
  • Cdens 0.17 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.58 Likely unique

Overview

â„šī¸
HSC 2910 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high 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.

Relatively close High extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Silver sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 261.934 -35.562 0.726 0.019 -0.947 1.944
Hunt & Reffert 2024 261.999 -35.521 0.721 -0.01 -0.95 -31.175
Cavallo et al. 2024 261.957 -35.711 0.724 – – –
Hunt & Reffert 2023 261.999 -35.521 0.721 -0.01 -0.95 -31.175

💡 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 – – – – – 267* – –
Cavallo et al. 2024 1.41 2.97 – 6 -0.170 – – –
Hunt & Reffert 2023 1.29 3.10 2.70 14 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2246 41.5 261.78 -35.93 0.78 0.1 -0.87 29.62 0.16

💡 Note: The % column shows the percentage of members that HSC 2910 shares with each listed object.

Visualization

â„šī¸