2016/04/26 by S. Ghazaryan, G. Alecian · 2 citations
Physics and Astronomy · #Stellar, planetary, and galactic studies #Astro and Planetary Science #Astronomy and Astrophysical Research #Stars #Physics #Multiplicity (mathematics) #Astrophysics #Abundance (ecology) #Effective temperature #Statistical analysis #Spectral line #Astronomy #Statistics #Biology #Ecology
paper · pdf · doi:10.1093/mnras/stw911
openalex publication_date 2016/04/26 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/30
To better understand the hot chemically peculiar group of HgMn stars, we have considered a compilation of a large number of recently published data obtained for these stars from spectroscopy. We compare these data to the previous compilation by Smith. We confirm the main trends of the abundance peculiarities, namely the increasing overabundances with increasing atomic number of heavy elements, and their large spread from star to star. For all the measured elements, we have looked for correlations between abundances and effective temperature (Teff). In addition to the known correlation for Mn, some other elements are found to show some connection between their abundances and Teff. We have also checked if multiplicity is a determinant parameter for abundance peculiarities determined for these stars. A statistical analysis using a Kolmogorov–Smirnov test shows that the abundances anomalies in the atmosphere of HgMn stars do not present significant dependence on the multiplicity.