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Pakmor R.
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Pakmor R.
Pakmor, Rüdiger
Pakmor, R.
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http://hub.abes.fr/edp/periodical/aa/2011/volume_528/issue_2011/aa15653-10/authorship/1
http://hub.abes.fr/edp/periodical/aa/2013/volume_554/issue_2013/aa20972-12/authorship/10
http://hub.abes.fr/edp/periodical/aa/2012/volume_548/issue_2012/aa19357-12/authorship/2
http://hub.abes.fr/oup/periodical/mnras/2010/volume_407/issue_4/101111j13652966201017106x/authorship/4
http://hub.abes.fr/edp/periodical/aa/2013/volume_554/issue_2013/aa20903-12/authorship/2
http://hub.abes.fr/edp/periodical/aa/2016/volume_589/issue_2016/aa28036-15/authorship/19
http://hub.abes.fr/edp/periodical/aa/2016/volume_593/issue_2016/aa28321-16/authorship/3
http://hub.abes.fr/edp/periodical/aa/2020/volume_635/issue_2020/aa37245-19/authorship/7
http://hub.abes.fr/edp/periodical/aa/2021/volume_650/issue_2021/aa40320-21/authorship/3
http://hub.abes.fr/edp/periodical/aa/2024/volume_686/issue_2024/aa49637-24/authorship/1
http://hub.abes.fr/edp/periodical/aa/2020/volume_642/issue_2020/aa38702-20/authorship/6
http://hub.abes.fr/edp/periodical/aa/2018/volume_618/issue_2018/aa33475-18/authorship/5
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Violent mergers of nearly equal-mass white dwarf as progenitors of subluminous Type Ia supernovae
Gamma-ray diagnostics of Type Ia supernovae
Do electron-capture supernovae make neutron stars?
Nucleosynthesis in thermonuclear supernovae with tracers: convergence and variable mass particles
Rotation of surviving companion stars after type Ia supernova explosions in the WD+MS scenario
The type Iax supernova, SN 2015H
White dwarf deflagrations for Type Iax supernovae: polarisation signatures from the explosion and companion interaction
Formation of sdB-stars via common envelope ejection by substellar companions
Revisiting the tension between fast bars and the ΛCDM paradigm
Three-dimensional simulations of the interaction between Type Ia supernova ejecta and their main sequence companions
Type Ia supernova explosion models are inherently multidimensional
Thermonuclear explosions of rapidly differentially rotating white dwarfs: Candidates for superluminous Type Ia supernovae?
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