Alessi 56

(MWSC 3047; DSH J1906.8+0935; GLIMPSE 19; Mercer 19)

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0.50 UTI
0.0
CN
1.0
Cdens
0.5
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members) 2.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.5 Moderately studied
  • Cdup 1.0 Unique

Overview

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Alessi 56 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by very high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is moderately studied in the literature.

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

Distant Very high extinction Intermediate age

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 286.715 9.597 0.28 -2.095 -5.436 –
He et al. 2023 286.722 9.592 0.258 -1.973 -5.357 –
Just et al. 2023 286.716 9.588 – – – –
SΓ‘nchez et al. 2020 286.717 9.583 – -1.805 -5.152 –
Bica et al. 2019 286.714 9.584 – – – –
Kharchenko et al. 2016 286.716 9.588 – – – –
Kharchenko et al. 2013 286.722 9.59 – 0.23 0.17 –
Kronberger et al. 2006 286.717 9.583 – – – –
Dias et al. 2002 286.717 9.583 – 0.23 0.17 –

πŸ’‘ 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
He et al. 2023 4.90 7.40 – 631 – – – –
Just et al. 2023 – – – 385 – 902 – –
Kharchenko et al. 2016 5.75 6.78 – 385 – – – –
Kharchenko et al. 2013 5.75 6.78 – 385 – – – –
Kronberger et al. 2006 3.90* 6.20* – – – – – –
Dias et al. 2002 3.90 6.20 – – – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
MCM 19 80.0 286.72 9.59 0.28 -2.07 -5.46 – 0.06

πŸ’‘ Note: The % column shows the percentage of members that Alessi 56 shares with each listed object.

Visualization

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