HSC 2698

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0.41 UTI
0.32
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.4 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2698 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Very high extinction Near-solar metallicity Young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 230.312 -57.115 0.364 -2.522 -2.994 -39.908
Hunt & Reffert 2024 230.311 -57.098 0.34 -2.508 -2.965 -40.306
Cavallo et al. 2024 230.323 -57.105 0.35 – – –
Hunt & Reffert 2023 230.311 -57.098 0.34 -2.508 -2.965 -40.306

💡 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 – – – – – 965* – –
Cavallo et al. 2024 2.08 5.05 – 81 -0.120 – – –
Hunt & Reffert 2023 2.58 5.57 2.39 55 – – – –

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

Visualization

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