46 citations · 72 across the 6 of their papers we have counts for
6 papers
Unlocking the Capabilities of Future High-Resolution X-ray Spectroscopy Missions Through Laboratory Astrophysics
Gabriele Betancourt-Martinez, Hiroki Akamatsu, Didier Barret +46
Thanks to high-resolution and non-dispersive spectrometers onboard future X-ray missions such as XRISM and Athena, we are finally poised to answer important questions about the for…
HST FUV monitoring of TW Hya
H. M. Günther, N. S. Brickhouse, A. K. Dupree +3
Classical T Tauri stars (CTTS) are young (< 10 Myr), cool stars that actively accrete matter from a disk. They show strong, broad and asymmetric, atomic FUV emission lines. Neither…
Structure and Dynamics of the Accretion Process and Wind in TW Hya
A. K. Dupree, N. S. Brickhouse, S. R. Cranmer +3
Time-domain spectroscopy of the classical accreting T Tauri star, TW Hya, covering a decade and spanning the far UV to the near-infrared spectral regions can identify the radiation…
Roles and Needs of Laboratory Astrophysics in NASA's Space and Earth Science Mission
Nancy Brickhouse, John Cowan, Paul Drake +9
Laboratory astrophysics and complementary theoretical calculations are the foundations of astronomy and astrophysics and will remain so into the foreseeable future. The mission ena…
Using Chandra/LETG spectra to probe stellar coronae
Gaitee A. J. Hussain, Nancy Brickhouse, Andrea K. Dupree +4
We probe the relationship between surface magnetic fields and the X-ray emitting corona in the rapidly rotating star AB Dor. Circularly polarised spectra have been inverted to prod…
X-ray Doppler Imaging of 44i Boo with Chandra
N. S. Brickhouse, A. K. Dupree, P. R. Young
Chandra High-Energy Transmission Grating observations of the bright eclipsing contact binary 44i Boo show X-ray line profiles which are Doppler-shifted by orbital motions. The X-ra…