Back to Search
Start Over
Star and Stellar Cluster Formation: ALMA-SKA Synergies
- Publication Year :
- 2015
-
Abstract
- Over the next decade, observations conducted with ALMA and the SKA will reveal the process of mass assembly and accretion onto young stars and will be revolutionary for studies of star formation. Here we summarise the capabilities of ALMA and discuss recent results from its early science observations. We then review infrared and radio variability observations of both young low-mass and high-mass stars. A time domain SKA radio continuum survey of star forming regions is then outlined. This survey will produce radio light-curves for hundreds of young sources, providing for the first time a systematic survey of radio variability across the full range of stellar masses. These light-curves will probe the magnetospheric interactions of young binary systems, the origins of outflows, trace episodic accretion on the central sources and potentially constrain the rotation rates of embedded sources.<br />Comment: 12 pages, 2 figures. To be published in the proceedings of "Advancing Astrophysics with the Square Kilometre Array", PoS(AASKA14) in press
Details
- Database :
- arXiv
- Publication Type :
- Report
- Accession number :
- edsarx.1504.03565
- Document Type :
- Working Paper