HSC 1388

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0.44 UTI
0.33
CN
1.0
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.1 [arcmin]
  • CN 0.33 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1388 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Relatively close High extinction 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 – 83.279 30.571 0.313 -0.038 -1.098 19.905
Zhang et al. 2024 83.275 30.569 – – – –
Hunt & Reffert 2024 83.275 30.569 0.315 -0.061 -1.125 20.191
Cavallo et al. 2024 83.273 30.568 0.324 – – –
Hunt & Reffert 2023 83.275 30.569 0.315 -0.061 -1.125 20.191

💡 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
Zhang et al. 2024 – – – – 0.080* – – –
Hunt & Reffert 2024 – – – – – 578* – –
Cavallo et al. 2024 2.73 3.62 – 251 0.260 – – –
Hunt & Reffert 2023 2.95 3.73 1.87 151 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3254 100.0 83.28 30.57 0.32 -0.04 -1.09 19.4 0.13

💡 Note: The % column shows the percentage of members that HSC 1388 shares with each listed object.

Visualization

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