113 citations · 621 across the 20 of their papers we have counts for
20 papers
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…
Search for Na in novae supported by a novel method for measuring femtosecond nuclear lifetimes
C. Fougères, F. de Oliveira Santos, J. José +58
Classical novae are thermonuclear explosions in stellar binary systems, and important sources of Al and Na. While gamma rays from the decay of the former radioisotope…
Experimentally well-constrained masses of P and S: Implications for studies of explosive binary systems
L. J. Sun, X. X. Xu, S. Q. Hou +58
The mass of P was predicted to impact the X-ray burst (XRB) model predictions of burst light curves and the composition of the burst ashes. To address the uncertainties and…
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…
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…
Classical-Nova Contribution to the Milky Way's Al Abundance: Exit Channel of the Key Al()Si Resonance
M. B. Bennett, C. Wrede, K. A. Chipps +21
Classical novae are expected to contribute to the 1809-keV Galactic -ray emission by producing its precursor Al, but the yield depends on the thermonuclear rate of the un…