Alessi 16

(MWSC 968)

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0.23 UTI
0.0
CN
0.26
Cdens
0.25
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 4.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.26 Loose
  • CC3 0.25 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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Alessi 16 is a sparse, loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.05 kpc) differs significantly from the median photometric distance (~2.09 kpc).

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

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.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 100.826 2.15 0.328 -0.258 1.502 70.834
Just et al. 2023 100.883 2.177 – – – –
Kharchenko et al. 2016 100.883 2.177 – – – –
Kharchenko et al. 2013 100.89 2.175 – -0.98 -2.14 50.3
Kronberger et al. 2006 100.896 2.173 – – – –
Dias et al. 2002 100.896 2.173 – -0.98 -2.14 –

💡 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– 2.09 1.94 – 447 – 16 – –
Just et al. 2023 – – – 447 – 16 – –
Kharchenko et al. 2016 2.09 1.94 – 447 – – – –
Kharchenko et al. 2013 2.09 1.94 – 447 – – – –
Dias et al. 2002 1.19 0.84 – 1122 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1659 80.0 100.81 2.12 0.33 -0.28 1.5 62.76 0.02

💡 Note: The % column shows the percentage of members that Alessi 16 shares with each listed object.

Visualization

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