Ruprecht 72

(MWSC 1591; OCL 737; ESO 371 22)

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0.24 UTI
0.0
CN
0.04
Cdens
0.38
CC3
0.4
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 0.4 Poorly studied
  • Cdup 1.0 Unique

Overview

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Ruprecht 72 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* 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 (~3.91 kpc) differs significantly from the median photometric distance (~2.50 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€“ 132.981 -37.639 0.256 -4.188 3.102 โ€“
Just et al. 2023 133.007 -37.607 โ€“ โ€“ โ€“ โ€“
Bica et al. 2019 133.011 -37.61 โ€“ โ€“ โ€“ โ€“
Kharchenko et al. 2016 133.007 -37.607 โ€“ โ€“ โ€“ โ€“
Kharchenko et al. 2013 133.012 -37.61 โ€“ -3.89 3.89 โ€“
Bukowiecki et al. 2011 133.0 -37.562 โ€“ โ€“ โ€“ โ€“
van den Bergh 2006 133.025 -37.6 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€“ 2.505 0.49 โ€“ 2512 โ€“ 238 โ€“ โ€“
Just et al. 2023 โ€“ โ€“ โ€“ 2512 โ€“ 101 โ€“ โ€“
Kharchenko et al. 2016 2.24 0.45 โ€“ 2512 โ€“ โ€“ โ€“ โ€“
Kharchenko et al. 2013 2.24 0.45 โ€“ 2512 โ€“ โ€“ โ€“ โ€“
Bukowiecki et al. 2012 โ€“ โ€“ โ€“ โ€“ โ€“ 376 โ€“ โ€“
Bukowiecki et al. 2011 2.77(1) 0.53 โ€“ 1413 โ€“ โ€“ โ€“ โ€“
van den Bergh 2006 3.02 0.74 โ€“ 1259 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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