HSC 2739

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0.48 UTI
0.38
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.38 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2739 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by very high extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Very high extinction Metal-rich 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 – 238.321 -51.815 0.403 -2.254 -3.465 -50.654
Hunt & Reffert 2024 238.311 -51.818 0.391 -2.272 -3.485 -36.895
Cavallo et al. 2024 238.348 -51.819 0.396 – – –
Hunt & Reffert 2023 238.311 -51.818 0.391 -2.272 -3.485 -36.895

💡 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 – – – – – 882* – –
Cavallo et al. 2024 2.07 5.49 – 65 0.540 – – –
Hunt & Reffert 2023 2.23 6.38 2.30 32 – – – –

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

Visualization

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