The onset of X-ray emission in young stellar objects

2006/11/16 by G. Giardino, Giovanna Giardino, F. Favata +4 · 1 citation
Physics and Astronomy · #Artificial intelligence #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Star Formation Studies #Class (philosophy) #Computer science #Optics #Physics #Protostar #Star formation #Stars #Stellar, planetary, and galactic studies #X-ray #Young stellar object #astro-ph

paper · pdf · doi:10.1051/0004-6361:20066424

Accepted for publication in A&A

arxiv created 2006/11/16 · openalex publication_date 2006/11/20 · arxiv updated 2009/12/01 · openalex created_date 2022/10/04 · openalex updated_date 2026/07/31

Abstract

Aims. To study the properties of X-ray emission from young stellar objects (YSOs) through their evolution from Class I to Class III and determine whether Class 0 protostars emit X-rays.

Citations

• Discovery of Extremely Embedded X‐Ray Sources in the R Coronae Australis Star‐forming Core
• Radio and X-ray variability of young stellar objects in theCoronetcluster
• Very Large Array 3.5 cm Continuum Sources in the Serpens Cloud Core
• The Origin of T Tauri X‐Ray Emission: New Insights from the Chandra Orion Ultradeep Project
• Discovery of X‐Rays from Class 0 Protostar Candidates in OMC‐3

Cited by

• ENERGETIC PROTONS, RADIONUCLIDES, AND MAGNETIC ACTIVITY IN PROTOSTELLAR DISKS