The solar–stellar connection

2004/09/07 by S. M. White · 18 citations
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Connection (principal bundle) #Gamma-ray bursts and supernovae #Physics #Sensitivity (control systems) #Square (algebra) #Stars #Stellar atmosphere #Stellar evolution #Stellar physics #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1016/j.newar.2004.09.014

published in New Astronomy Reviews 48(11-12), 1319-1326 (Elsevier BV) · to appear in "Science with the Square Kilometer Array," eds. C. Carilli and S. Rawlings, New Astronomy Reviews (Elsevier: Amsterdam)

arxiv created 2004/09/07 · openalex publication_date 2004/12/01 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

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.

Citations

• Radio Emission fromROSAT‐discovered Young Stars in and around Taurus‐Auriga
• A Multiwavelength Perspective of Flares on HR 1099: 4 Years of Coordinated Campaigns
• Stellar Radio Astronomy: Probing Stellar Atmospheres from Protostars to Giants
• A Giant Flare on a T Tauri Star Observed at Millimeter Wavelengths