Dr. habil. Isabelle Cherchneff-Parrinello
Philosophisch-Naturwissenschaftliche Fakultät
Departement Physik


Departement Physik
Klingelbergstrasse 82
4056 Basel


Cherchneff, I. und Sarangi, A. (2017) «New Insights on What, Where, and How Dust Forms in Evolved Stars», in Miroshnichenko, A., Zharikov, S., Korv cáková, D., und Wolf, M. (Hrsg.) The B[e] Phenomenon: Forty Years of Studies 3rd International Conference on Studies of the B[e] Phenomenon. Astronomical Society of the Pacific (Astronomical Society of the Pacific Conference Series, 508), S. 57. Verfügbar unter: http://www.aspbooks.org/a/volumes/article_details/?paper_id=37983.   edoc
Kamiński, T., Müller, H. S. P., Schmidt, M. R., Cherchneff, I., Wong, K. T., Brünken, S., Menten, K. M., Winters, J. M., Gottlieb, C. A. und Patel, N. A. (2017) «An observational study of dust nucleation in Mira (o Ceti). II. Titanium oxides are negligible for nucleation at high temperatures», Astronomy and Astrophysics. EDP Sciences, 599, S. A59. doi: 10.1051/0004-6361/201629838.   edoc | Open Access
Gobrecht, D., Cherchneff, I., Sarangi, A., Plane, J. M. C. und Bromley, S. T. (2016) «Dust formation in the oxygen-rich AGB star IK Tauri», Astronomy and Astrophysics. EDP Sciences, 585, S. A6. doi: 10.1051/0004-6361/201425363.   edoc | Open Access
Titel Status
Forming cosmic dust in low- and high-mass, evolved stars Abgeschlossen
"Aspects of Chemical Evolution" An Inter-CRP EuroGenesis Mini- Workshop Abgeschlossen
Dust synthesis in evolved stellar winds: a local diagnostic for the identification of dust providers in the early universe. Abgeschlossen