Hydrogen burning of $^{29}$Si and its impact on presolar stardust grains from classical novae

Autor: Lori Downen, Christian Iliadis, Art Champagne, Thomas Clegg, Alain Coc, Jordi José

Publikováno v: UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
Digital.CSIC. Repositorio Institucional del CSIC
instname

Presolar stardust grains found in primitive meteorites are believed to retain the isotopic composition of stellar outflows at the time of grain condensation. Therefore, laboratory measurements of their isotopic ratios represent sensitive probes for i

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::86383c1b10b94d2cae4aa8f4f763f3a4
http://arxiv.org/abs/2202.11568