HXHWL 42

(H21OC 42)

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0.19 UTI
0.26
CN
0.13
Cdens
0.38
CC3
0.1
Clit
1.0
Cdup
Core radius and density 2.0 [pc], 0.7 [pc-2]
  • CN 0.26 Poorly populated
  • Cdens 0.13 Very loose
  • CC3 0.38 Low quality
  • Clit 0.1 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HXHWL 42 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 122.335 -35.598 0.888 -4.735 3.007 18.151
Hunt & Reffert 2024 122.322 -35.659 0.891 -4.765 2.993 11.784
Cavallo et al. 2024 122.367 -35.599 0.892 – – –
Hunt & Reffert 2023 122.322 -35.659 0.891 -4.765 2.993 11.784
He et al. 2022 122.244 -35.542 0.874 -4.669 3.011 –
He et al. 2021 122.332 -35.568 0.86 -4.78 2.97 –

💡 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] Bfrac BSS
UCC 99999– 1.095 0.62 0.81 137 0.277 156 – –
Hunt & Reffert 2024 1.06 0.43 0.81 137 – 156(1) – –
Cavallo et al. 2024 1.13 0.62 – 219 0.320 – – –
Hunt & Reffert 2023 1.06 0.43 0.81 137 – – – –
He et al. 2022 – 0.85 – 63 – – – –
He et al. 2021 1.20 0.89 – 91 0.233 – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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