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astro-ph.SR2026
New NanoSIMS Multielement Isotope Data Reveal CO Novae As Key Sources Of 13C-rich Presolar Silicon Carbide Grains
Jordi José, Nan Liu, Conel M. O'D. Alexander +1
We present new multielement NanoSIMS isotopic measurements (C, N, Si, Mg-Al, Ti, and Ni) for four putative nova SiC grains and 79 AB SiC grains from the Murchison meteorite to reas…
astro-ph.SR2014★ 5 cited
Strength of the E_R = 127 keV, 26Al(p,g)27Si resonance
A. Parikh, J. Jose, A. Karakas +2
We examine the impact of the strength of the E_R = 127 keV, 26Al(p,g)27Si resonance on 26Al production in classical nova explosions and asymptotic giant branch (AGB) stars. Thermon…
astro-ph.SR2014
Classical novae and type I X-ray bursts: challenges for the 21st century
A. Parikh, J. Jose, G. Sala
Classical nova explosions and type I X-ray bursts are the most frequent types of thermonuclear stellar explosions in the Galaxy. Both phenomena arise from thermonuclear ignition in…