Aims. We present a detailed study of X-ray absorption in the local interstellar medium by analyzing the X-ray spectra of 24 galactic sources obtained with the Chandra High Energy Transmission Grating Spectrometer and the XMM-Newton Reflection Grating Spectrometer. Methods. By modeling the continuum with a simple broken power-law and by implementing the new ISMab
All observations of Galactic X-ray binaries are affected by absorption from gas and dust in the inte...
We present recent results on high‐resolution X‐ray absorption measurements of the interstellar mediu...
We present the first X-ray detection of resonant absorption from warm/hot local gas either in our Ga...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2001.Includes bibliographi...
We find resolved interstellar O K, Ne K, and Fe L absorption spectra in the Chandra Low Energy Trans...
Understanding the chemistry of the interstellar medium (ISM) is fundamental for the comprehension of...
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...
We present an X-ray absorption line spectroscopic study of the large-scale hot interstellar medium (...
Context. The diffuse interstellar medium (ISM) is an integral part of the evolution of the entire Ga...
Aims. The interstellar medium (ISM) has a multiphase structure characterized by gas, dust, and molec...
Aims. The interstellar medium (ISM) has a multiphase structure characterized by gas, dust, and molec...
(Abbrv.) We present high-resolution spectroscopy of the oxygen K-shell interstellar absorption edge ...
<p>The chemical evolution of the Universe embraces aspects that reachdeep into modern astrophysics a...
High resolution X-ray spectra of the Reflection Grating Spectrometer (RGS) on board the XMM satellit...
All observations of Galactic X-ray binaries are affected by absorption from gas and dust in the inte...
We present recent results on high‐resolution X‐ray absorption measurements of the interstellar mediu...
We present the first X-ray detection of resonant absorption from warm/hot local gas either in our Ga...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2001.Includes bibliographi...
We find resolved interstellar O K, Ne K, and Fe L absorption spectra in the Chandra Low Energy Trans...
Understanding the chemistry of the interstellar medium (ISM) is fundamental for the comprehension of...
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...
We present an X-ray absorption line spectroscopic study of the large-scale hot interstellar medium (...
Context. The diffuse interstellar medium (ISM) is an integral part of the evolution of the entire Ga...
Aims. The interstellar medium (ISM) has a multiphase structure characterized by gas, dust, and molec...
Aims. The interstellar medium (ISM) has a multiphase structure characterized by gas, dust, and molec...
(Abbrv.) We present high-resolution spectroscopy of the oxygen K-shell interstellar absorption edge ...
<p>The chemical evolution of the Universe embraces aspects that reachdeep into modern astrophysics a...
High resolution X-ray spectra of the Reflection Grating Spectrometer (RGS) on board the XMM satellit...
All observations of Galactic X-ray binaries are affected by absorption from gas and dust in the inte...
We present recent results on high‐resolution X‐ray absorption measurements of the interstellar mediu...
We present the first X-ray detection of resonant absorption from warm/hot local gas either in our Ga...