scholarly journals Using Multiwavelength Variability to Explore the Connection among X-Ray Emission, the Far-ultraviolet H2 Bump, and Accretion in T Tauri Stars

2019 ◽  
Vol 876 (2) ◽  
pp. 121 ◽  
Author(s):  
C. C. Espaillat ◽  
C. Robinson ◽  
S. Grant ◽  
M. Reynolds
Keyword(s):  
T Tauri Stars ◽  
X Ray ◽  
T Tauri ◽  
Far Ultraviolet ◽  
Multiwavelength Variability

T Tauri Stars: The X-Ray Connection

1999 ◽  
pp. 119-120
Author(s):  
V. M. Costa ◽  
M. T. V. T. Lago
Keyword(s):  
T Tauri Stars ◽  
X Ray ◽  
T Tauri

X-ray sources in regions of star formation. III - Naked T Tauri stars associated with the Taurus-Auriga complex

1988 ◽  
Vol 96 ◽  
pp. 297 ◽  
Author(s):  
Frederick M. Walter ◽  
A. Brown ◽  
R. D. Mathieu ◽  
P. C. Myers ◽  
F. J. Vrba
Keyword(s):  
Star Formation ◽  
T Tauri Stars ◽  
X Ray ◽  
T Tauri

Einstein Observations of T Tauri Stars in Taurus-Auriga. I. Properties of X-Ray Emission

1995 ◽  
Vol 446 ◽  
pp. 331 ◽  
Author(s):  
F. Damiani ◽  
G. Micela ◽  
S. Sciortino ◽  
F. R., Jr. Harnden
Keyword(s):  
T Tauri Stars ◽  
X Ray ◽  
T Tauri

X-ray observations of T Tauri stars

1980 ◽  
Vol 242 ◽  
pp. L163 ◽  
Author(s):  
G. F. Gahm
Keyword(s):  
T Tauri Stars ◽  
X Ray ◽  
T Tauri

scholarly journals X-ray emission of multiple T Tauri stars in Taurus

2001 ◽  
Vol 369 (3) ◽  
pp. 971-980 ◽  
Author(s):  
B. König ◽  
R. Neuhäuser ◽  
B. Stelzer
Keyword(s):  
T Tauri Stars ◽  
X Ray ◽  
T Tauri

scholarly journals X-ray Flare Rate of T Tauri Stars in Taurus

1995 ◽  
Vol 151 ◽  
pp. 216-217
Author(s):  
R. Neuhäuser ◽  
Th. Preibisch
Keyword(s):  
Star Formation ◽  
Main Sequence ◽  
T Tauri Stars ◽  
Medium Size ◽  
Late Type ◽  
Large Sample ◽  
X Ray ◽  
T Tauri ◽  
Sky Survey ◽  
Low Mass

AbstractWe study the X-ray emission of several hundred (young, low-mass, late-type, pre-main sequence) T Tauri stars (TTS) in the Taurus T association, a nearby well-studied region of ongoing star formation. We report on X-ray emission variability of TTS as observed with the flux-limited ROSAT All-Sky Survey (RASS). Since RASS observations are spatially unbiased, we can investigate the X-ray flare rate of TTS on a large sample. We find that large flares are very rare (once per year), while medium-size flares can occur once in ∼ 40 days.

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

2007 ◽  
Vol 468 (2) ◽  
pp. 443-462 ◽  
Author(s):  
A. Telleschi ◽  
M. Güdel ◽  
K. R. Briggs ◽  
M. Audard ◽  
L. Scelsi
Keyword(s):  
High Resolution ◽  
T Tauri Stars ◽  
X Ray ◽  
T Tauri

Absorption of X-ray emission of t tauri stars by circumstellar material

1995 ◽  
Vol 224 (1-2) ◽  
pp. 93-96 ◽  
Author(s):  
Ralph Neuh�user ◽  
Michael F. Sterzik ◽  
J�rgen H. M. M. Schmitt
Keyword(s):  
T Tauri Stars ◽  
X Ray ◽  
Circumstellar Material ◽  
T Tauri

scholarly journals Non thermal emission from T Tauri stars

2010 ◽  
Vol 6 (S275) ◽  
pp. 404-405
Author(s):  
María V. del Valle ◽  
Gustavo E. Romero
Keyword(s):  
Main Sequence ◽  
Thermal Emission ◽  
High Energy ◽  
Magnetic Activity ◽  
T Tauri Stars ◽  
Main Sequence Stars ◽  
High Energy Radiation ◽  
X Ray ◽  
T Tauri ◽  
Low Mass

AbstractT Tauri stars are low mass, pre-main sequence stars. These objects are surrounded by an accretion disk and present strong magnetic activity. T Tauri stars are copious emitters of X-ray emission which belong to powerful magnetic reconnection events. Strong magnetospheric shocks are likely outcome of massive reconnection. Such shocks can accelerate particles up to relativistic energies through Fermi mechanism. We present a model for the high-energy radiation produced in the environment of T Tauri stars. We aim at determining whether this emission is detectable. If so, the T Tauri stars should be very nearby.

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