Fast transition between classical and weak lined T Tauri stars due to external UV dissipation [PDF]
, 2007 The discovery of optical jets immersed in the strong UV radiation field of the Rosette Nebula sheds new light on, but meanwhile poses challenges to, the study of externally irradiated jets. The jet systems in the Rosette are found to have a high state of
J.Z. Li, Travis A. Rector
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The Magnetic Fields of Classical T Tauri Stars [PDF]
, 2007 We report new magnetic field measurements for 14 classical T Tauri stars (CTTSs). We combine these data with one previous field determination in order to compare our observed field strengths with the field strengths predicted by magnetospheric accretion ...
Christopher M. Johns‐Krull
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Profiles of Strong Permitted Lines in Classical T Tauri Stars [PDF]
, 2000 We present a spectral analysis of 30 T Tauri stars observed with the Hamilton echelle spectrograph over more than a decade. One goal is to test magnetospheric accretion model predictions.
S. H. P. Alencar, Gibor Basri
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Role of local absorption on the X-ray emission from MHD accretion shocks in classical T Tauri stars [PDF]
EPJ Web of Conferences, 2014 Accretion processes onto classical T Tauri stars (CTTSs) are believed to generate shocks at the stellar surface due to the impact of supersonic downflowing plasma.
Bonito +8 more
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The Astrophysical JournalAn accurate estimation of the continuum excess emission from accretion spots and inner circumstellar disk regions is crucial for a proper derivation of fundamental stellar parameters in accreting systems.
Facundo Pérez Paolino +4 more
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On the formation of H line emission around classical T Tauri stars [PDF]
Monthly Notices of the Royal Astronomical Society, 2006 Timothy Harries
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Spectral variability of classical T Tauri stars accreting in an unstable regime [PDF]
Monthly Notices of the Royal Astronomical Society, 2013 Ryuichi Kurosawa, M. M. Romanova
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Photometric and spectroscopic study of five pre-main sequence stars in the vicinity of NGC 7129 [PDF]
Serbian Astronomical Journal, 2019 We present results from long-term optical photometric and spectroscopic observations of five pre-main sequence stars, located in the vicinity of the bright nebula NGC 7129.
Semkov E.H., Ibryamov S.I., Peneva S.P.
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Dust Around T Tauri Stars [PDF]
Journal of Astronomy and Space Sciences, 2011 To reproduce the multiple broad peaks and the fine spectral features in the spectral energy distributions (SEDs) of T Tauri stars, we model dust around T Tauri stars using a radiative transfer model for multiple isothermal circumstellar dust shells. We
Kyung-Won Suh, Young-Joo Kwon
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Multidimensional models of hydrogen and helium emission line profiles for classical T Tauri stars: method, tests and examples [PDF]
Monthly Notices of the Royal Astronomical Society, 2011 Ryuichi Kurosawa +2 more
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