Title: Uncovering the ingredients for planet formation

Title: Protostellar jets and planet-forming disks: Witnessing the formation of Solar System analogues with interferometry. Issue

We consider each of these parameters: disk structure (i.e. tracing the evolution from massive protostellar disks to T Tauri disks, to transitional disks, and debris disks), stellar

Tyrone van der Meer, founder of The Notorious IBE (IBE), an international breaking event, and Angelo Martinus, founder of the urban scene in Eindhoven and initiator of EMOVES, an

This interpretation requires that (1) the HCN/H 2 O flux ratio is sensitive to the relative masses of HCN and H 2 O in the molecular emission region; (2) submillimeter disk masses are

De sterkte van het 10 micron silicaatfeature van T Tauri-sterren wordt niet alleen bepaald door de grootte van het stof in de schijf. De meter-barrière, die aangeeft dat rotsblokken

The similarities in structure (e.g. scale height of the gas disk, radial exponential tail, surface den- sity power-law index) and dust composition (small and large grains

Moreover, (2) while in the 1D case the accretion rate onto the planet is limited by the efficiency that gas can accrete through the circumplanetary disk, the limiting factor in the

Nonetheless, the current limited spectral surface brightness sensitivity of ALMA restricts the study of the crucial gas component of planet formation to a handful of the most