HSC 2737

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0.29 UTI
0.41
CN
0.68
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.2 [arcmin]
  • CN 0.41 Poorly populated
  • Cdens 0.68 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2737 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate 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 – 240.417 -53.879 0.351 -2.564 -3.44 -15.303
Hunt & Reffert 2024 240.441 -53.867 0.361 -2.546 -3.417 -15.371
Cavallo et al. 2024 240.433 -53.876 0.359 – – –
Hunt & Reffert 2023 240.441 -53.867 0.361 -2.546 -3.417 -15.371

💡 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 – – – – – 511* – –
Cavallo et al. 2024 2.62 2.90 – 48 -0.380 – – –
Hunt & Reffert 2023 2.54 2.49 2.30 96 – – – –

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

Visualization

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