2011/02/06 by P. Benaglia, Paula Benaglia, Benaglia, Paula
Engineering · Physics and Astronomy · #Astro and Planetary Science #Electrical and Electromagnetic Research #FOS: Physical sciences #Muon and positron interactions and applications #Solar and Stellar Astrophysics (astro-ph.SR) #astro-ph.SR
paper · pdf · doi:10.48550/arxiv.1102.1147
To appear in Rev.Mex. Astron.Astrof., 6 pages, 7 figs (Invited review)
arxiv created 2011/02/06 · openalex publication_date 2011/02/06 · arxiv updated 2011/02/08 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/04
The study of the formation of massive stars presents complex challenges from both theoretical and observational points of view. The initial phases of evolution, for instance, remain almost hidden except at radio and IR wavelengths. In this article, after stating some of the problems of massive star formation, the role of radio observations to disclose the involved physics is discussed. Historical observational findings are briefly outlined, and the connection between low energy and high energy aspects of the phenomenon is addressed. Finally, data availability in the form of some new surveys is reported.