Ruprecht 158

(MWSC 1592; OCL 736; ESO 371 23)

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0.22 UTI
0.0
CN
0.04
Cdens
0.38
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad) 0.2 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.04 Very loose
  • CC3 0.38 Low quality
  • Clit 0.35 Poorly studied
  • Cdup 1.0 Unique

Overview

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Ruprecht 158 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~5.05 kpc) differs significantly from the median photometric distance (~2.72 kpc).

โš ๏ธ 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.

Dias et al. (2002)
Field fluctuation (Vรกzquez, R. A. et al. 2010, A&A 511, 38); cat V3.5 (Jan 2016)

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999โ€“ 133.09 -37.6 0.198 -3.166 2.993 โ€“
Just et al. 2023 133.105 -37.552 โ€“ โ€“ โ€“ โ€“
Bica et al. 2019 133.106 -37.56 โ€“ โ€“ โ€“ โ€“
Kharchenko et al. 2016 133.105 -37.552 โ€“ โ€“ โ€“ โ€“
Kharchenko et al. 2013 133.11 -37.555 โ€“ -1.3 2.32 โ€“
Bukowiecki et al. 2011 133.108 -37.56 โ€“ โ€“ โ€“ โ€“
van den Bergh 2006 133.075 -37.567 โ€“ โ€“ โ€“ โ€“

๐Ÿ’ก 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 99999โ€“ 2.72 0.985 โ€“ 1413 โ€“ 276 โ€“ โ€“
Just et al. 2023 โ€“ โ€“ โ€“ 1413 โ€“ 276 โ€“ โ€“
Kharchenko et al. 2016 2.72 1.23 โ€“ 1413 โ€“ โ€“ โ€“ โ€“
Kharchenko et al. 2013 2.72 1.23 โ€“ 1413 โ€“ โ€“ โ€“ โ€“
Bukowiecki et al. 2011 2.70(1) 0.59 โ€“ 1778 โ€“ โ€“ โ€“ โ€“
van den Bergh 2006 4.17 0.74 โ€“ 1585 โ€“ โ€“ โ€“ โ€“

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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