HSC 1358

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0.08 UTI
0.0
CN
0.43
Cdens
0.25
CC3
0.25
Clit
0.36
Cdup
Radius (P>50% members) 5.0 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.43 Loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.36 Possibly duplicate

Overview

â„šī¸
HSC 1358 is a sparse, loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Low extinction Near-solar metallicity Intermediate age

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 – 81.409 33.902 0.465 0.263 -2.072 –
Zhang et al. 2024 81.402 33.896 – – – –
Hunt & Reffert 2024 81.402 33.896 0.468 0.252 -2.086 –
Cavallo et al. 2024 81.434 33.891 0.47 – – –
Hunt & Reffert 2023 81.402 33.896 0.468 0.252 -2.086 –

💡 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 – – – – -0.351* – – –
Hunt & Reffert 2024 – – – – – 107* – –
Cavallo et al. 2024 2.32 0.43 – 200 -0.160 – – –
Hunt & Reffert 2023 1.93 0.81 1.04 28 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4099 88.0 81.4 33.9 0.47 0.28 -2.07 – 0.03
LP 19 64.0 81.33 33.86 0.45 0.24 -2.05 – 0.17

💡 Note: The % column shows the percentage of members that HSC 1358 shares with each listed object.

Visualization

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