5 citations · 5 across the 2 of their papers we have counts for
6 papers
Structure and Dynamics of Stellar Winds in High-mass X-ray Binaries
M. Sako, S. M. Kahn, F. Paerels +4
A review of spectroscopic results obtained from Chandra High Energy Transmission Grating Spectrometer and XMM-Newton Reflection Grating Spectrometer observations of several wind-fe…
Soft X-ray Spectra of Seyfert 2 Galaxies
Masao Sako, Ali Kinkhabwala, Steven M. Kahn +6
High resolution spectroscopic observations of Seyfert galaxies with Chandra and XMM-Newton allows us to study the detailed ionization and thermal structures of the X-ray absorbing/…
Soft X-ray Spectroscopy of NGC 1068 with XMM-Newton RGS and Chandra LETGS
A. Kinkhabwala, M. Sako, E. Behar +7
We present high-resolution soft-X-ray spectra of the prototypical Seyfert 2 galaxy, NGC 1068, taken with XMM-Newton RGS and Chandra LETGS. Its rich emission-line spectrum is domina…
Soft X-ray Spectroscopy of Seyfert 2 Galaxies
A. Kinkhabwala, M. Sako, E. Behar +6
Soft X-ray spectroscopy of Seyfert 2 galaxies offers perhaps the best method to probe the possible connection between AGN activity and star formation. Obscuration of powerful radia…
Confronting atomic data with Fe L-shell spectra of stellar coronae
E. Behar, J. Cottam, J. R. Peterson +5
It is common to suggest the uncertainties in the atomic data for explaining difficulties that arise in interpreting astrophysical x-ray spectra. The atomic data for the Fe L-shell…
A physically consistent model for X-ray emission by Seyfert 2 galaxies demonstrated on NGC 1068
E. Behar, A. Kinkhabwala, M. Sako +5
Preliminary analysis of the X-ray spectrum of NGC 1068 obtained by the RGS spectrometer on board XMM-Newton is presented. A physically consistent model is developed in order to qua…