High-resolution X-ray spectroscopy of T Tauri stars in the Taurus-Auriga complex

2006/11/01 by A. Telleschi, M. Güdel, M. Guedel +3 · 4 citations
Physics and Astronomy · #Accretion (finance) #Accretion disc #Astro and Planetary Science #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Emission spectrum #Herbig Ae/Be star #K-type main-sequence star #Spectroscopy #Stars #T Tauri star #astro-ph

paper · pdf · doi:10.1051/0004-6361:20066193

22 pages, 9 figures, to be published in A&A, to appear in a special section/issue dedicated to the XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST)

arxiv created 2006/11/01 · openalex publication_date 2007/02/05 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context.Differences have been reported between the X-ray emission of accreting and non-accreting stars. Some observations have suggested that accretion shocks could be responsible for part of the X-ray emission in classical T Tauri stars (CTTS).

Citations

• The first high-resolution X-ray spectrum of a Herbig star: AB Aurigae
• Collisional Plasma Models with APEC/APED: Emission-Line Diagnostics of Hydrogen-like and Helium-like Ions
• Observations of X-ray emission from T Tauri stars
• Accretion in Young Stellar/Substellar Objects
• On the sizes of stellar X-ray coronae
• The XMM-Newton extended survey of the Taurus molecular cloud (XEST)
• X-ray accretion signatures in the close CTTS binary V4046 Sagittarii
• X-ray emission from young stars in Taurus-Auriga-Perseus: Luminosity functions and the rotation -activity -age -relation
• A statistical analysis of X-ray variability in pre-main sequence objects of the Taurus molecular cloud
• The Coronae of AB Doradus and V471 Tauri: Primordial Angular Momentum versus Tidal Spin‐up
• The Origin of T Tauri X‐Ray Emission: New Insights from the Chandra Orion Ultradeep Project
• X-ray astronomy of stellar coronae

Cited by

• X-ray emitting MHD accretion shocks in classical T Tauri stars. Case for moderate to high plasma-β values
• X‐rays from young stars: A summary of highlights from the XMM‐Newton Extended Survey of the Taurus Molecular Cloud (XEST)
• The XMM-Newton Optical Monitor survey of the Taurus molecular cloud
• X-rays from T Tauri: a test case for accreting T Tauri stars