The Formation of Star and Planetary Systems: New Results from Spitzer

TL;DR

This paper reviews new observational findings from Spitzer on the evolution of protostars and protoplanetary disks, highlighting their implications for planet formation and disk dissipation processes.

Contribution

It presents novel observational data from Spitzer that enhance understanding of protostellar evolution and disk development in star-forming regions.

Findings

Insights into the structure of protoplanetary disks

Observations of episodic accretion events

Implications for planet formation processes

Abstract

Protoplanetary disks are thought to be the birth places of planetary systems. The formation and the subsequent evolution of protoplanetary disks are regulated by the star formation process, which begins with the collapse of a cloud core to form a central protostar surrounded by a disk and an overlying envelope. In the protostellar phase, most of the envelope material is transferred onto the star through the disk during episodic, high accretion events. The initial conditions for planet formation in protoplanetary disks are likely set by the details of these processes. In this contribution, I will review some of the new observational results from Spitzer on protostellar evolution and the structure and evolution of protoplanetary disks surrounding young stars in the nearby star forming regions. The implications of these results for planet formation and eventual disk dissipation are discussed.