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Constraining the dark matter content of NGC 1291 using hydrodynamic gas response simulations
Online Contents | 2017| -
Constraining the dark matter content of NGC 1291 using hydrodynamic gas response simulations
Online Contents | 2016| -
A close look at secular evolution: Boxy/peanut bulges reduce gas inflow to the central kiloparsec
Free accessArXiv | 2016| -
Constraining the dark matter content of NGC 1291 using hydrodynamic gas response simulations
Free accessArXiv | 2016| -
Breaking the disc-halo degeneracy in NGC 1291 using hydrodynamic simulations
Free accessArXiv | 2016| -
Searching for a kinematic signature of the moderately metal-poor stars in the Milky Way bulge using N-body simulations
Free accessEDP Sciences | 2018| -
The disc origin of the Milky Way bulge
Free accessDissecting the chemo-morphological relations using N-body simulations and APOGEEEDP Sciences | 2018| -
Bars and boxy/peanut bulges in thin and thick discs
Free accessI. Morphology and line-of-sight velocities of a fiducial modelEDP Sciences | 2017| -
The disc origin of the Milky Way bulge: On the necessity of the thick disc
Free accessArXiv | 2019| -
Disk origin of the Milky Way bulge: the necessity of the thick disk
Free accessEDP Sciences | 2019| -
What the Milky Way bulge reveals about the initial metallicity gradients in the disc
Free accessEDP Sciences | 2017| -
What the Milky Way bulge reveals about the initial metallicity gradients in the disc
Free accessArXiv | 2017| -
Chemical Characterization of the Inner Galactic bulge:North-South Symmetry
Free accessArXiv | 2018| -
The dual origin of the Galactic thick disc and halo from the gas-rich Gaia-Enceladus Sausage merger
Free accessBASE | 2020|Contributors: Fragkoudi F. -
Revisiting the tension between fast bars and the ΛCDM paradigm
Free accessBASE | 2021|Contributors: Fragkoudi F.
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