We find resolved interstellar O K, Ne K, and Fe L absorption spectra in the Chandra X-Ray Observatory Low-Energy Transmission Grating Spectrometer (LETGS) spectrum of the low-mass X-ray binary X0614+091. We measure the column densities in O and Ne and find direct spectroscopic constraints on the chemical state of the interstellar O. These measurements probably probe a low-density line of sight through the Galaxy, and we discuss the results in the context of our knowledge of the properties of interstellar matter in regions between the spiral arms
We present detailed analyses of oxygen K absorption in the interstellar medium (ISM) using four high...
We present an X-ray absorption line spectroscopic study of the large-scale hot interstellar medium (...
Aims. The interstellar medium (ISM) has a multiphase structure characterized by gas, dust, and molec...
We find resolved interstellar O K, Ne K, and Fe L absorption spectra in the Chandra Low Energy Trans...
We present high-resolution spectroscopy of the neon K-shell and iron L-shell interstellar absorption...
X-ray absorption spectroscopy provides a powerful tool in determining the metal abundances in variou...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2004.Includes bibliographi...
Context. The diffuse interstellar medium (ISM) is an integral part of the evolution of the entire Ga...
(Abbrv.) We present high-resolution spectroscopy of the oxygen K-shell interstellar absorption edge ...
Context. Low-mass X-ray binaries (LMXBs) are a natural workbench to study accretion disk phenomena a...
We present a study of the C K-edge using high-resolution LETGS Chandraspectra of four novae during t...
Using a hydrodynamic simulation of a cold dark matter universe with a cosmological constant, we inve...
Aims. The interstellar medium (ISM) has a multiphase structure characterized by gas, dust, and molec...
Aims. We present a detailed study of X-ray absorption in the local interstellar medium by analyzing ...
We use four Chandra gratings spectra of the neutron star low-mass X-ray binary 4U 1820–30 to better ...
We present detailed analyses of oxygen K absorption in the interstellar medium (ISM) using four high...
We present an X-ray absorption line spectroscopic study of the large-scale hot interstellar medium (...
Aims. The interstellar medium (ISM) has a multiphase structure characterized by gas, dust, and molec...
We find resolved interstellar O K, Ne K, and Fe L absorption spectra in the Chandra Low Energy Trans...
We present high-resolution spectroscopy of the neon K-shell and iron L-shell interstellar absorption...
X-ray absorption spectroscopy provides a powerful tool in determining the metal abundances in variou...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2004.Includes bibliographi...
Context. The diffuse interstellar medium (ISM) is an integral part of the evolution of the entire Ga...
(Abbrv.) We present high-resolution spectroscopy of the oxygen K-shell interstellar absorption edge ...
Context. Low-mass X-ray binaries (LMXBs) are a natural workbench to study accretion disk phenomena a...
We present a study of the C K-edge using high-resolution LETGS Chandraspectra of four novae during t...
Using a hydrodynamic simulation of a cold dark matter universe with a cosmological constant, we inve...
Aims. The interstellar medium (ISM) has a multiphase structure characterized by gas, dust, and molec...
Aims. We present a detailed study of X-ray absorption in the local interstellar medium by analyzing ...
We use four Chandra gratings spectra of the neutron star low-mass X-ray binary 4U 1820–30 to better ...
We present detailed analyses of oxygen K absorption in the interstellar medium (ISM) using four high...
We present an X-ray absorption line spectroscopic study of the large-scale hot interstellar medium (...
Aims. The interstellar medium (ISM) has a multiphase structure characterized by gas, dust, and molec...