LISC 1273

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0.30 UTI
0.0
CN
0.25
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.25 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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LISC 1273 is a sparse, loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a significant percentage of members with 2 later reported entries. See table with shared members information.

Distant Moderate extinction Near-solar metallicity Very 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 – 177.92 -63.311 0.255 -5.539 0.719 –
Hunt & Reffert 2024 177.786 -63.314 0.249 -5.516 0.712 –
Cavallo et al. 2024 177.841 -63.296 0.249 – – –
Hunt & Reffert 2023 177.786 -63.314 0.249 -5.516 0.712 –
Li et al. 2022 177.898 -63.317 0.252 -5.615 0.709 –

💡 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
Hunt & Reffert 2024 – – – – – 474* – –
Cavallo et al. 2024 3.87 2.17 – 16 0.270 – – –
Hunt & Reffert 2023 3.80 2.01 2.49 15 – – – –
Li et al. 2022 2.51 1.57 – 100 -0.419 – 0.49 –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3992 72.0 177.92 -63.3 0.25 -5.52 0.72 -20.26 0.05
CWWDL 873 4.0 177.89 -63.28 0.27 -5.67 0.73 – 0.08

💡 Note: The % column shows the percentage of members that LISC 1273 shares with each listed object.

Visualization

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