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


Departement Physik
Klingelbergstrasse 82
4056 Basel


Cherchneff, I. and Sarangi, A. (2017) “New Insights on What, Where, and How Dust Forms in Evolved Stars”, in Miroshnichenko, A., Zharikov, S., Korv cáková, D., and Wolf, M. (eds.) 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), p. 57. Available at: 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. and 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, p. A59. doi: 10.1051/0004-6361/201629838.   edoc | Open Access
Gobrecht, D., Cherchneff, I., Sarangi, A., Plane, J. M. C. and Bromley, S. T. (2016) “Dust formation in the oxygen-rich AGB star IK Tauri”, Astronomy and Astrophysics. EDP Sciences, 585, p. A6. doi: 10.1051/0004-6361/201425363.   edoc | Open Access
Title Status
Forming cosmic dust in low- and high-mass, evolved stars Complete
"Aspects of Chemical Evolution" An Inter-CRP EuroGenesis Mini- Workshop Complete
Dust synthesis in evolved stellar winds: a local diagnostic for the identification of dust providers in the early universe. Complete