Alessi 55

(FSR 1080; MWSC 1038)

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0.14 UTI
0.0
CN
0.05
Cdens
0.12
CC3
0.26
Clit
1.0
Cdup
Core radius and density 2.0 [pc], 0.2 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.05 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.26 Poorly studied
  • Cdup 1.0 Unique

Overview

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Alessi 55 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~2.65 kpc) differs significantly from the median photometric distance (~1.75 kpc).

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.

Bica et al. (2019)
List of clusters and alike reported by B. Alessi.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 104.546 0.88 0.378 -1.052 1.973 –
Just et al. 2023 104.558 0.885 – – – –
Bica et al. 2019 104.572 0.868 – – – –
Dib et al. 2018 104.565 0.884 – – – –
Sampedro et al. 2017 104.567 0.865 – -0.35 2.41 –
Joshi et al. 2016 104.565 0.884 – – – –
Kharchenko et al. 2016 104.558 0.885 – – – –
Dias et al. 2014 104.567 0.865 – 0.27 -0.15 –
Kharchenko et al. 2013 104.565 0.884 – -1.99 -4.54 –
Froebrich et al. 2007 104.567 0.865 – – – –
Dias et al. 2002 104.567 0.865 – -1.99 -4.54 –

💡 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– 1.75 1.77 – 234 – 104 – –
Just et al. 2023 – – – 234 – 104 – –
Dib et al. 2018 1.75 – – 234 – – – –
Joshi et al. 2016 1.75 1.77 – 234 – – – –
Kharchenko et al. 2016 1.75 1.77 – 234 – – – –
Kharchenko et al. 2013 1.75 1.77 – 234 – – – –
Dias et al. 2002 1.75 1.77 – 234 – – – –

Visualization

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