Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Stars, Astronomy, Metallicity, and Supernova.
Chemical evolution with radial mixing redux: a detailed model for formation and evolution of the Milky Way
The messy death of a multiple star system and the resulting planetary nebula as observed by JWST
The complex stellar system M 22: confirming abundance variations with high precision differential measurements
The GALAH survey: tracing the Galactic disc with open clusters
How Magnetic Activity Alters What We Learn from Stellar Spectra
Tidal Interactions between Binary Stars Can Drive Lithium Production in Low-mass Red Giants
Direct Capture Cross Section and the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi>E</mml:mi></mml:mrow><mml:mrow><mml:mi>p</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn>71</mml:mn></mml:mrow></mml:math> and 105 keV Resonances in the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi>Ne</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>
Origin of meteoritic stardust unveiled by a revised proton-capture rate of 17O
Detailed homogeneous abundance studies of 14 Galactic<i>s</i>-process enriched post-AGB stars: In search of lead (Pb)
18 Sco: A SOLAR TWIN RICH IN REFRACTORY AND NEUTRON-CAPTURE ELEMENTS. IMPLICATIONS FOR CHEMICAL TAGGING
ON THE SOURCE OF THE DUST EXTINCTION IN TYPE Ia SUPERNOVAE AND THE DISCOVERY OF ANOMALOUSLY STRONG Na I ABSORPTION
THE IMPACT OF UPDATED Zr NEUTRON-CAPTURE CROSS SECTIONS AND NEW ASYMPTOTIC GIANT BRANCH MODELS ON OUR UNDERSTANDING OF THE<i>S</i>PROCESS AND THE ORIGIN OF STARDUST
Post-AGB stars in the SMC as tracers of stellar evolution: the extreme s-process enrichment of the 21 <i>μ</i>m star J004441.04-732136.4