We find resolved interstellar O K, Ne K, and Fe L absorption spectra in the Chandra Low Energy Transmission Grating Spectrometer 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 a high-resolution (=D 500) X-ray spectrum of the bright quasar H1821+643 (z 0:297), o...
We present a comprehensive study of interstellar X-ray extinction using the extensive Chandra supern...
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 X-Ray Observator...
We present high-resolution spectroscopy of the neon K-shell and iron L-shell interstellar absorption...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2004.Includes bibliographi...
X-ray absorption spectroscopy provides a powerful tool in determining the metal abundances in variou...
Context. Low-mass X-ray binaries (LMXBs) are a natural workbench to study accretion disk phenomena a...
Aims. We present a detailed study of X-ray absorption in the local interstellar medium by analyzing ...
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 ...
Understanding the chemistry of the interstellar medium (ISM) is fundamental for the comprehension of...
Aims. The interstellar medium (ISM) has a multiphase structure characterized by gas, dust, and molec...
Using a hydrodynamic simulation of a cold dark matter universe with a cosmological constant, we inve...
We present the first X-ray detection of resonant absorption from warm/hot local gas either in our Ga...
We present a high-resolution (=D 500) X-ray spectrum of the bright quasar H1821+643 (z 0:297), o...
We present a comprehensive study of interstellar X-ray extinction using the extensive Chandra supern...
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 X-Ray Observator...
We present high-resolution spectroscopy of the neon K-shell and iron L-shell interstellar absorption...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2004.Includes bibliographi...
X-ray absorption spectroscopy provides a powerful tool in determining the metal abundances in variou...
Context. Low-mass X-ray binaries (LMXBs) are a natural workbench to study accretion disk phenomena a...
Aims. We present a detailed study of X-ray absorption in the local interstellar medium by analyzing ...
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 ...
Understanding the chemistry of the interstellar medium (ISM) is fundamental for the comprehension of...
Aims. The interstellar medium (ISM) has a multiphase structure characterized by gas, dust, and molec...
Using a hydrodynamic simulation of a cold dark matter universe with a cosmological constant, we inve...
We present the first X-ray detection of resonant absorption from warm/hot local gas either in our Ga...
We present a high-resolution (=D 500) X-ray spectrum of the bright quasar H1821+643 (z 0:297), o...
We present a comprehensive study of interstellar X-ray extinction using the extensive Chandra supern...
Aims. The interstellar medium (ISM) has a multiphase structure characterized by gas, dust, and molec...