CWNU 1281

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0.33 UTI
0.35
CN
0.22
Cdens
0.5
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 1.1 [N/pc2]
  • CN 0.35 Poorly populated
  • Cdens 0.22 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1281 is a poorly populated, very loose object of intermediate 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, young cluster (see Parameters). It was recently reported in the literature.

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

Palma et al. (2025)
Part of multiple system G40, along with HSC_1641, CWNU_158, HSC_1636 and Collinder_104.

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 99999– 100.676 4.726 0.643 -1.964 0.794 –
Zhang et al. 2024 100.645 4.728 – – – –
Hunt & Reffert 2024 100.645 4.728 0.641 -1.959 0.798 –
Cavallo et al. 2024 100.633 4.7 0.639 – – –
Hunt & Reffert 2023 100.645 4.728 0.641 -1.959 0.798 –
He et al. 2023 100.62 4.753 0.644 -1.972 0.816 –

💡 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– 1.48 0.95 0.87 58 0.051 170 – –
Zhang et al. 2024 – – – – -0.089(1) – – –
Hunt & Reffert 2024 – – – – – 170(1) – –
Cavallo et al. 2024 1.51 0.95 – 58 0.190 – – –
Hunt & Reffert 2023 1.47 0.91 0.87 69 – – – –
He et al. 2023 1.48 1.10 – 40 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1636 5.7 99.85 4.94 0.64 -2.04 0.75 28.99 0.05

💡 Note: The % column shows the percentage of members that CWNU 1281 shares with each listed object.

Visualization

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