Add to ORKGOB stars with strong radiation-driven stellar winds and large-scale magnetic fields generate strong and hard X-ray emission via the Magnetically Channeled Wind Shock (MCWS) mechanism. In this brief paper, I describe four separate X-ray diagnostics of the MCWS mechanism in OB stars, with applications to the prototype young O star, theta-1 Ori C
The X-ray properties of twenty ~1 Myr old O, B, and A stars of the Orion Trapezium are examined with...
Magnetically confined winds of early-type stars are expected to be sources of bright and hard X-rays...
Nearly all types of massive stars are known to display X-ray emission at some level. Tremendous insi...
Young O stars are strong, hard, and variable X-ray sources, properties which strongly affect their c...
The magnetic activity of solar-type and low-mass stars is a well known source of coronal X-ray emiss...
The magnetic activity of solar-type and low-mass stars is a well known source of coronal X-ray emiss...
We report on four Chandra grating observations of the oblique magnetic rotator theta(1) Ori C (O5.5 ...
High-resolution X-ray spectra of high-mass stars and low-mass T-Tauri stars obtained during the firs...
Magnetic fields have been frequently invoked as a likely source of variability and confinement of th...
Over the last decade, large-scale, organized (generally dipolar) magnetic fields with a strength bet...
A subset (∼ 10%) of massive stars present strong, globally ordered (mostly dipolar) magnetic fields....
Young O stars are strong, hard, and variable X-ray sources, properties which strongly a®ect their ci...
peer reviewedWe observed NGC 1624-2, the O-type star with the largest known magnetic field (B[SUB]p[...
X-rays give direct evidence of instabilities, time-variable structure, and shock heating in the wind...
X-ray emission from stars much more massive than the Sun was discovered only 35 years ago. Such star...
The X-ray properties of twenty ~1 Myr old O, B, and A stars of the Orion Trapezium are examined with...
Magnetically confined winds of early-type stars are expected to be sources of bright and hard X-rays...
Nearly all types of massive stars are known to display X-ray emission at some level. Tremendous insi...
Young O stars are strong, hard, and variable X-ray sources, properties which strongly affect their c...
The magnetic activity of solar-type and low-mass stars is a well known source of coronal X-ray emiss...
The magnetic activity of solar-type and low-mass stars is a well known source of coronal X-ray emiss...
We report on four Chandra grating observations of the oblique magnetic rotator theta(1) Ori C (O5.5 ...
High-resolution X-ray spectra of high-mass stars and low-mass T-Tauri stars obtained during the firs...
Magnetic fields have been frequently invoked as a likely source of variability and confinement of th...
Over the last decade, large-scale, organized (generally dipolar) magnetic fields with a strength bet...
A subset (∼ 10%) of massive stars present strong, globally ordered (mostly dipolar) magnetic fields....
Young O stars are strong, hard, and variable X-ray sources, properties which strongly a®ect their ci...
peer reviewedWe observed NGC 1624-2, the O-type star with the largest known magnetic field (B[SUB]p[...
X-rays give direct evidence of instabilities, time-variable structure, and shock heating in the wind...
X-ray emission from stars much more massive than the Sun was discovered only 35 years ago. Such star...
The X-ray properties of twenty ~1 Myr old O, B, and A stars of the Orion Trapezium are examined with...
Magnetically confined winds of early-type stars are expected to be sources of bright and hard X-rays...
Nearly all types of massive stars are known to display X-ray emission at some level. Tremendous insi...