Alessi 144

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0.29 UTI
0.0
CN
0.34
Cdens
0.5
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 15.3 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.34 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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Alessi 144 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.
Close Low extinction Near-solar metallicity Intermediate age

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 – 112.615 5.642 1.179 -2.667 -1.563 10.814
Zhang et al. 2024 112.592 5.717 – – – –
Hunt & Reffert 2024 112.592 5.717 1.154 -2.653 -1.497 19.145
Cavallo et al. 2024 112.646 5.666 1.159 – – –
Hunt & Reffert 2023 112.592 5.717 1.154 -2.653 -1.497 19.145
Bica et al. 2019 112.605 5.486 – – – –

💡 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 – – – – -0.210* – – –
Hunt & Reffert 2024 – – – – – 84* – –
Cavallo et al. 2024 0.87 0.24 – 74 0.280 – – –
Hunt & Reffert 2023 0.81 0.08 0.35 128 – – – –

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

Visualization

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