Add to ORKGThis thesis presents new insights of protoplanetary disk evolution. It focuses on the characterisation of several elements in the earliest phases of planet formation in protoplanetary disks: the connection between the SED and disk gaps (Chapters 2, 3 and 4), PAHs in the gas flows in disk gaps (Chapter 5) and dust processing of forsterite in evolving protoplanetary disks (Chapter 6).LKBF, Leiden observatoryUBL - phd migration 201
Context. Characterizing the evolution of protoplanetary disks is necessary to improve our understand...
The scope of this thesis is to investigate the structure and evolution of protoplanetary disk. High ...
The protoplanetary disks seen around Herbig Ae stars eventually dissipate leaving just a tenuous deb...
A large diversity of exoplanetary systems has been found, but it is still unclear what drives this d...
Stars form as a result of gravitational collapse of an interstellar molecular cloud. In the process,...
The planets, comets, asteroids... all objects in the Solar system have become from a single disc of ...
Nascent envelope disk structures around protostars play a crucial role in the process of star and pl...
This article summarizes a Splinter Session at the Cool Stars XV conference in St. Andrews with 3 rev...
Tijdens mijn doctoraat heb ik protoplanetaire schijven bestudeerd: de schijven van gas en stof rond ...
The first steps of planet formation imply that dust grows from interstellar-like particles to planet...
The early evolutionary stages of a pre-main sequence star are characterised by the formation of a d...
Protoplanetary disks are the essential link between molecular clouds and planetary systems. Protopla...
Young stars are surrounded by massive, rotating disks of dust and gas, which supply a reservoir of m...
The work presented in this thesis is based on ALMA surveys of protoplanetary disks in three star-for...
This thesis discusses the physical and chemical processes than influence the composition...
Context. Characterizing the evolution of protoplanetary disks is necessary to improve our understand...
The scope of this thesis is to investigate the structure and evolution of protoplanetary disk. High ...
The protoplanetary disks seen around Herbig Ae stars eventually dissipate leaving just a tenuous deb...
A large diversity of exoplanetary systems has been found, but it is still unclear what drives this d...
Stars form as a result of gravitational collapse of an interstellar molecular cloud. In the process,...
The planets, comets, asteroids... all objects in the Solar system have become from a single disc of ...
Nascent envelope disk structures around protostars play a crucial role in the process of star and pl...
This article summarizes a Splinter Session at the Cool Stars XV conference in St. Andrews with 3 rev...
Tijdens mijn doctoraat heb ik protoplanetaire schijven bestudeerd: de schijven van gas en stof rond ...
The first steps of planet formation imply that dust grows from interstellar-like particles to planet...
The early evolutionary stages of a pre-main sequence star are characterised by the formation of a d...
Protoplanetary disks are the essential link between molecular clouds and planetary systems. Protopla...
Young stars are surrounded by massive, rotating disks of dust and gas, which supply a reservoir of m...
The work presented in this thesis is based on ALMA surveys of protoplanetary disks in three star-for...
This thesis discusses the physical and chemical processes than influence the composition...
Context. Characterizing the evolution of protoplanetary disks is necessary to improve our understand...
The scope of this thesis is to investigate the structure and evolution of protoplanetary disk. High ...
The protoplanetary disks seen around Herbig Ae stars eventually dissipate leaving just a tenuous deb...