Research into the fundamental topic of star formation has come of age in recent years, with the era of major spaced-based facilities such as the Herschel, Chandra, and Spitzer observatories. Such facilities have aided in the investigation of important questions in star formation, such as: how is the formation and evolution of stellar clusters effected by their initial conditions and environment? what are the effects of cluster environment on the processing of circumstellar material of young stars? and more recently with Herschel, what is the relation of core mass to the initial mass function and the filamentary structure observed in molecular clouds? Though we have made great headway in recent times, yet these puzzles remain unsolved.

The future missions and telescope facilities, expected to come online in the next decade, will open new avenues of research, and help answer some of these outstanding questions while also providing new avenues of inquiry and new puzzles to pursue. With Gaia and ALMA due to come online over the next two years, and JWST and SPICA planned to replace the current space missions in the coming decade, this workshop aims to discuss such missions and how they will impact future research on the frontiers of star formation.

The workshop will bring together young researchers at postdoctoral and PhD level with established researchers in the field to share their current work and to foster new collaborations for future projects. Overviews of currently operating and planned future missions will be provided and complimented by review talks on the major scientific questions under discussion. Ample time for open discussion will be provided.

There will be four broad sessions: