HSC 1502

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0.02 UTI
0.0
CN
0.28
Cdens
0.25
CC3
0.25
Clit
0.12
Cdup
Radius (P>50% members) 7.3 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.28 Loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.12 Likely duplicate

Overview

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HSC 1502 is a sparse, loose object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

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

Relatively close Moderate extinction Near-solar metallicity Young

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 – 94.492 22.644 0.527 0.45 -1.675 –
Zhang et al. 2024 94.474 22.632 – – – –
Hunt & Reffert 2024 94.474 22.632 0.527 0.433 -1.676 –
Cavallo et al. 2024 94.506 22.674 0.528 – – –
Hunt & Reffert 2023 94.474 22.632 0.527 0.433 -1.676 –

💡 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 – – – – -0.056* – – –
Hunt & Reffert 2024 – – – – – 226* – –
Cavallo et al. 2024 2.01 2.00 – 112 0.560 – – –
Hunt & Reffert 2023 1.83 2.17 1.51 51 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14032 88.0 94.5 22.65 0.53 0.42 -1.66 -32.33 0.05
UBC 1306 72.0 94.62 22.88 0.53 0.45 -1.62 -1.83 0.21
FSR 0891 24.0 94.38 22.45 0.54 0.41 -1.71 – 0.19
OC 0311 8.0 94.37 22.39 0.57 0.47 -1.74 – 0.12

💡 Note: The % column shows the percentage of members that HSC 1502 shares with each listed object.

Visualization

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