Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Monash University Melbourne
Sterrekundig Instituut, Utrecht University, The Netherlands
Sterrekundig Instituut, University of Utrecht, Postbus 80000, 3508 TA Utrecht, The Netherlands for Stellar and Planetary Astrophysics, School of Mathematical Sciences, Monash University, Clayton, VIC 3800; Sterrekundig Instituut, University of Utrecht, Postbus 80 000, 3508 TA Utrecht, The Netherlands
Department of Mathematics, Monash University, Clayton 3168, Victoria, Australia
Sterrekundig Instituut Utrecht, Postbus 80000, 3508 TA Utrecht, The Netherlands; Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK
Astronomical Institute, Princetonplein 5, 3584 CC Utrecht, The Netherlands
University of Cambridge, Institute of Astronomy, Cambridge CB3 0HA, UK
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB30HA, United Kingdom
Institute of Astronomy, University of Cambridge, Madingley Rd, Cambridge CB3 0HA, United Kingdom
University of Utrecht, Utrecht, Netherlands
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
Institute of Astronomy, Madingley Road, Cambridge, CB3 0DS, United Kingdom
Utrecht, Monash
U Utrecht
University of Cambridge
IoA, University of Cambridge, UK
Sterrekundig Instituut, Universiteit Utrecht, P.O. Box 80000, 3508 TA Utrecht, The Netherlands; Centre for Stellar and Planetary Astrophysics, School of Mathematical Sciences, Monash University, Victoria 3800, Australia
Astronomical Institute, University of Utrecht, Postbus 80000, 3508 TA Utrecht, Netherlands.
Centre for Stellar and Planetary Astrophysics, Monash University, Clayton 3800, Victoria, Australia
Dipartimento di Fisica Generale, Università di Torino, Via P. Giuria 1, I-10125 Torino, Italy Instituut, University of Utrecht, Postbus 80000, 3508 TA Utrecht, The Netherlands. Institute, University of Utrecht, Postbus 80000, 3
/s processing in post-AGB and CH stars at low metallicity
26Al and 60Fe yields from AGB stars
A Massive AGB Star as Source of Short-Lived Nuclei in the Early Solar System
A New Astrophysical Interpretation of the Si and Ti Isotopic Compositions of Mainstream SiC Grains from Primitive Meteorites
Al and Ti Isotopic Ratios of Presolar SiC Grains of Type Z
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