Ruprecht 89

(MWSC 1808; OCL 812; ESO 127 21)

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0.26 UTI
0.0
CN
0.2
Cdens
0.12
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members) 5.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.2 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.5 Moderately studied
  • Cdup 1.0 Unique

Overview

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Ruprecht 89 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by low extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~2.47 kpc) differs significantly from the median photometric distance (~0.75 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.

Close Low extinction Low mass 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 – 157.134 -58.164 0.405 -7.066 2.571 –
Just et al. 2023 157.102 -58.131 – – – –
Bica et al. 2019 157.109 -58.18 – – – –
Kharchenko et al. 2016 157.102 -58.131 – – – –
Dias et al. 2014 157.108 -58.183 – -4.12 1.3 –
Kharchenko et al. 2013 157.107 -58.135 – -3.75 5.13 –
Piskunov et al. 2008 157.116 -58.136 – – – –
Kharchenko et al. 2005 157.11 -58.14 – -6.82 4.36 –
Kharchenko et al. 2003 157.06 -58.13 – -5.86 4.04 –

💡 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
Just et al. 2023 – – – 955 – 10 – –
Kharchenko et al. 2016 0.75 0.12 – 955 – – – –
Kharchenko et al. 2013 0.75 0.12 – 955 – – – –
Piskunov et al. 2008 0.75 0.12 – 955 – – – –
Kharchenko et al. 2005 0.75 0.12 – 955 – – – –
Kharchenko et al. 2003 0.91 0.31 – – – – – –

Visualization

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