The Solar--Stellar Connection

Abstract

Stars have proven to be surprisingly prolific radio sources and the added sensitivity of the Square Kilometer Array will lead to advances in many directions. This chapter discusses prospects for studying the physics of stellar atmospheres and stellar winds across the HR diagram.

to appear in "Science with the Square Kilometer Array," eds. C. Carilli and S. Rawlings, New Astronomy Reviews (Elsevier: Amsterdam)

References in corpus (5)

• Measured Mass Loss Rates of Solar-like Stars as a Function of Age and Activity
• Stellar Radio Astronomy. Probing Stellar Atmospheres from Protostars to Giants
• A Giant Outburst at Millimeter Wavelengths in the Orion Nebula
• A Multi-Wavelength Perspective of Flares on HR 1099: Four Years of Coordinated Campaigns
• A giant flare on a t tauri star observed at millimeter wavelengths

Cited by in corpus (12)

• EMU: Evolutionary Map of the Universe
• Radio emission and mass loss rate limits of four young solar-type stars
• The MicroJy and NanoJy Radio Sky: Source Population and Multi-wavelength Properties
• First Detection of Thermal Radio Emission from Solar-Type Stars with the Karl G. Jansky Very Large Array
• SCORPIO: A deep survey of Radio Emission from the stellar life-cycle
• Detection of Alpha Centauri at radio wavelengths: chromospheric emission and search for star-planet interaction
• EMISSA -- Exploring Millimeter Indicators of Solar-Stellar Activity I. The Initial mm-cm Main Sequence Star Sample
• Detection of thermal radio emission from a single coronal giant
• EMISSA -- Exploring Millimetre Indicators of Solar-Stellar Activity II. Towards a robust indicator of stellar activity
• Radio stars of the SKA
• First Detection of Radio Emission Associated with a Classical Cepheid
• Role of non-thermal processes in the quiescent and active millimeter spectrum of a young M dwarf