HSC 2913

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0.39 UTI
0.44
CN
1.0
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.0 [arcmin]
  • CN 0.44 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2913 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~3.74 kpc) differs significantly from the median photometric distance (~2.84 kpc).

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Relatively close Very high extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 262.584 -35.471 0.267 -1.18 -2.843 159.225
Hunt & Reffert 2024 262.581 -35.476 0.278 -1.127 -2.825 64.269
Cavallo et al. 2024 262.592 -35.467 0.269 – – –
Hunt & Reffert 2023 262.581 -35.476 0.278 -1.127 -2.825 64.269

💡 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 – – – – – 2368* – –
Cavallo et al. 2024 2.61 5.47 – 151 0.270 – – –
Hunt & Reffert 2023 3.07 5.49 2.67 207 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3218 100.0 262.59 -35.47 0.28 -1.18 -2.86 -5.37 0.27

💡 Note: The % column shows the percentage of members that HSC 2913 shares with each listed object.

Visualization

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