activity
20002014
most citedChandra HETGS Multi-Phase Spectroscopy of the Young Magnetic O Star theta^1 Orionis C

200 citations · 358 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2014★ 31 cited

Control and diagnosis of temperature, density, and uniformity in x-ray heated iron/magnesium samples for opacity measurements

T. Nagayama, J. E. Bailey, G. Loisel +5

Experimental tests are in progress to evaluate the accuracy of the modeled iron opacity at solar interior conditions, in particular to better constrain the solar abundance problem…

physics.plasm-ph2012★ 20 cited

One-dimensional radiation-hydrodynamic simulations of imploding spherical plasma liners with detailed equation-of-state modeling

J. S. Davis, S. C. Hsu, I. E. Golovkin +2

This work extends the one-dimensional radiation-hydrodynamic imploding spherical argon plasma liner simulations of T. J. Awe et al. [Phys. Plasmas 18, 072705 (2011)] by using a det…

astro-ph2007

Short-N characteristic radiative transfer method in 2D cylindrical RZ coordinates

Nicolas A. Pereyra, Joseph J. MacFarlane, Pamela R. Woodruff +2

We present a new radiative transfer method Short-N Characteristics that is a hybrid between the standard long characteristic methods and the standard short characteristic methods.…

astro-ph2005★ 200 cited

Chandra HETGS Multi-Phase Spectroscopy of the Young Magnetic O Star theta^1 Orionis C

Marc Gagne, Mary E. Oksala, David H. Cohen +5

We report on four Chandra grating observations of the oblique magnetic rotator theta^1 Ori C (O5.5 V) covering a wide range of viewing angles with respect to the star's 1060 G dipo…

astro-ph2004★ 23 cited

High Resolution X-ray Spectra of the Brightest OB Stars in the Cygnus OB2 Association

W. L. Waldron, J. P. Cassinelli, N. A. Miller +2

The Cygnus OB2 Association contains some of the most luminous OB stars in our Galaxy, the brightest of which are also among the most luminous in X-rays. We have obtained a Chandra…

astro-ph2002★ 2 cited

X ray emission line profile modeling of hot stars

Roban H. Kramer, Stephanie K. Tonnesen, David H. Cohen +3

The launch of high-spectral-resolution x-ray telescopes (Chandra, XMM) has provided a host of new spectral line diagnostics for the astrophysics community. In this paper we discuss…