Work

X-rays from jet-driving protostars and T Tauri stars

Year: 2006

Type: article

Abstract: Aims.We study jet-driving protostars and T Tau stars to characterize their X-ray emission. We seek soft spectral components that may be due to shock emission, and search for soft, shock-induced emission displaced from the stellar position.

Source: Astronomy and Astrophysics

DOI: 10.1051/0004-6361:20065736

Authors: M. Güdel, A. Telleschi, M. Audard, S. L. Skinner, K. R. Briggs, F. Palla, C. Dougados

Institutions: Paul Scherrer Institute, Columbia University, University of Colorado Boulder, Arcetri Astrophysical Observatory, Centre National de la Recherche Scientifique, Université Joseph Fourier, Institut de Planétologie et d'Astrophysique de Grenoble

Language: English

Topic: Astrophysics and Star Formation Studies

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: bronze

Funders: National Science Foundation, National Aeronautics and Space Administration, California Institute of Technology, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung

Awards: Röntgenastronomie stellarer Atmosphären, X-ray astronomy of stellar atmospheres

OpenAlex ID: W2020204680

FWCI: 4.26

Cites: 95

Cited by: 75

Related to: 10