Zamponi, Joaquin (2023): Comparing real and synthetic observations of protostellar disks. Dissertation, LMU München: Fakultät für Physik |
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Zamponi_Joaquin.pdf 22MB |
Abstract
Nascent envelope disk structures around protostars play a crucial role in the process of star and planet formation. As ALMA reveals unprecedented details of the envelope, disk, and outflow structures in nearby protostellar systems, a consistent interpretation for these observations remains absent, instead, highly simplified models are often adopted to partially fit the observed features. In this project, we aim to generate more realistic synthetic observations of the nascent protostellar disk and envelope system, using existing radiation and non-ideal magnetohydrodynamic simulations of protostellar collapse and disk formation. The main goal of the project is to provide multi-facet interpretation of the current continuum and polarization observations of protostellar sources at their earliest stages, and offer more realistic constraints on the dust growth in the early protoplanetary disks.
Dokumententyp: | Dissertationen (Dissertation, LMU München) |
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Keywords: | astronomy, star formation, protostellar disks, protoplanetary disks, observations, numerical simulations |
Themengebiete: | 500 Naturwissenschaften und Mathematik
500 Naturwissenschaften und Mathematik > 530 Physik |
Fakultäten: | Fakultät für Physik |
Sprache der Hochschulschrift: | Englisch |
Datum der mündlichen Prüfung: | 18. Juli 2023 |
1. Berichterstatter:in: | Caselli, Paola |
MD5 Prüfsumme der PDF-Datei: | e69d1f8e1823b2cf32e38e2396143888 |
Signatur der gedruckten Ausgabe: | 0001/UMC 29979 |
ID Code: | 32616 |
Eingestellt am: | 27. Oct. 2023 11:41 |
Letzte Änderungen: | 27. Oct. 2023 11:41 |