Evangelia Ntormousi
Affiliations: | Scuola Normale Superiore, Pisa, Toscana, Italy |
Area:
AstrphysicsGoogle:
"Evangelia Ntormousi"Mean distance: (not calculated yet)
Cross-listing: Astronomy Tree
Parents
Sign in to add mentor| Andreas Burkert | grad student | 2012 | Ludwig-Maximilian-University of Munich |
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Publications
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| Ntormousi E, Tassis K, Del Sordo F, et al. (2020) A dynamo amplifying the magnetic field of a Milky-Way-like galaxy Astronomy & Astrophysics. 641: A165 |
| Korkidis G, Pavlidou V, Tassis K, et al. (2020) Turnaround radius of galaxy clusters in N-body simulations Astronomy & Astrophysics. 639: A122 |
| Ntormousi E. (2018) Magnetic fields in massive spirals: The role of feedback and initial conditions Astronomy and Astrophysics. 619 |
| Ntormousi E, Dawson JR, Hennebelle P, et al. (2017) The role of magnetic fields in the structure and interaction of supershells Astronomy and Astrophysics. 599: 1-15 |
| Fierlinger KM, Burkert A, Ntormousi E, et al. (2016) Stellar feedback efficiencies: Supernovae versus stellar winds Monthly Notices of the Royal Astronomical Society. 456: 710-730 |
| Ntormousi E, Hennebelle P, André P, et al. (2016) The effect of ambipolar diffusion on low-density molecular ISM filaments Astronomy and Astrophysics. 589 |
| Ntormousi E, Hennebelle P. (2015) Shell instability of a collapsing dense core Astronomy and Astrophysics. 574 |
| Ntormousi E, Burkert A, Fierlinger K, et al. (2011) Formation Of Cold Filamentary Structure From Wind-Blown Superbubbles The Astrophysical Journal. 731: 13 |
| Ntormousi E, Sommer-Larsen J. (2010) Hot gas haloes around disc galaxies: O vii column densities from galaxy formation simulations Monthly Notices of the Royal Astronomical Society. 409: 1049-1056 |