scholarly journals High‐Resolution X‐Ray Spectroscopy of the Interstellar Medium. II. Neon and Iron Absorption Edges

2006 ◽  
Vol 648 (2) ◽  
pp. 1066-1078 ◽  
Author(s):  
Adrienne M. Juett ◽  
Norbert S. Schulz ◽  
Deepto Chakrabarty ◽  
Thomas W. Gorczyca
2010 ◽  
Author(s):  
J. S. Kaastra ◽  
C. P. de Vries ◽  
E. Costantini ◽  
J. W. A. den Herder ◽  
A. J. J. Raassen ◽  
...  

1983 ◽  
Vol 101 ◽  
pp. 289-293
Author(s):  
R. Petre ◽  
C. R. Canizares ◽  
P. F. Winkler ◽  
F. D. Seward ◽  
R. Willingale ◽  
...  

We present soft X-ray photomosaic images of two supernova remnants, Puppis A and IC 443, constructed from a series of exposures by the Einstein imaging instruments. The complex morphologies displayed in these images reflect the interaction between “middle-aged” supernova remnants and various components of the interstellar medium. Surface brightness variations across Puppis A suggest that inhomogeneities on scales from 0.2 to 30 pc are present in the interstellar medium, while the structure of IC 443 is apparently dominated by the interaction between the remnant and a giant molecular cloud.


2009 ◽  
Vol 5 (S267) ◽  
pp. 362-369
Author(s):  
Keiichi Wada

AbstractIn order to clarify the physics of AGN feedback and feeding, we need to understand the interstellar medium (ISM) in the central several tens of parsecs in galaxies where our observational and theoretical knowledge is relatively poor. Here we discuss feedback processes due to strong far UV and X-ray radiation, as well as the dynamical effect of a supermassive black hole (SMBH) based on new high-resolution numerical simulations of the ISM in the central R ≤ 32 pc region around a SMBH at the center of a galaxy.


2010 ◽  
Vol 521 ◽  
pp. A79 ◽  
Author(s):  
C. Pinto ◽  
J. S. Kaastra ◽  
E. Costantini ◽  
F. Verbunt

2002 ◽  
Vol 09 (01) ◽  
pp. 387-391 ◽  
Author(s):  
A. J. NELSON ◽  
T. VAN BUUREN ◽  
C. BOSTEDT ◽  
K. I. SCHAFFERS ◽  
LOU TERMINELLO

X-ray photoemission and X-ray photoabsorption were used to study the composition and the electronic structure of ytterbium-doped strontium fluoroapatite (Yb:S-FAP). High resolution photoemission measurements on the valence band electronic structure were used to evaluate the density of occupied states of this fluoroapatite. Element-specific density of unoccupied electronic states in Yb:S-FAP was probed by X-ray absorption spectroscopy (XAS) at the Yb 4d ( N 4,5-edge), Sr 3d ( M 4,5-edge), P 2p ( L 2,3-edge), F 1s and O 1s (K-edges) absorption edges. These results provide the first measurements of the electronic structure and surface chemistry of this material.


1982 ◽  
Vol 258 ◽  
pp. 22 ◽  
Author(s):  
R. Petre ◽  
G. A. Kriss ◽  
P. F. Winkler ◽  
C. R. Canizares

2004 ◽  
Vol 612 (1) ◽  
pp. 308-318 ◽  
Author(s):  
Adrienne M. Juett ◽  
Norbert S. Schulz ◽  
Deepto Chakrabarty

1986 ◽  
Vol 121 (2) ◽  
pp. 321-332
Author(s):  
J. Y. Deschamps ◽  
R. Rocchia ◽  
A. Tarrius

2009 ◽  
Vol 696 (2) ◽  
pp. 1418-1430 ◽  
Author(s):  
Yangsen Yao ◽  
Norbert. S. Schulz ◽  
Ming F. Gu ◽  
Michael A. Nowak ◽  
Claude. R. Canizares

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