X-rays from protostellar jets: emission from continuous flows

2006/10/17 by R. Bonito, S. Orlando, G. Peres +3 · 2 citations
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Cosmic Phenomena #Astrophysics and Star Formation Studies #Context (archaeology) #Geology #Physics #Quantum, superfluid, helium dynamics #astro-ph

paper · pdf · doi:10.1051/0004-6361:20065236

13 pages, 10 figures, accepted for publication in Astronomy and Astrophysics

arxiv created 2006/10/17 · openalex publication_date 2006/11/13 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Context.Recently X-ray emission from protostellar jets has been detected with both XMM-Newton and Chandra satellites, but the physical mechanism which can give rise to this emission is still unclear.

Citations

• X‐Rays from HH 80, HH 81, and the Central Region
• FLASH: An Adaptive Mesh Hydrodynamics Code for Modeling Astrophysical Thermonuclear Flashes
• Crushing of interstellar gas clouds in supernova remnants. I. The role of thermal conduction and radiative losses

Cited by

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• A Comparison of the X-Ray Properties of FU Ori-type Stars to Generic Young Stellar Objects