X-Ray Ionization and the Chemistry of the Orion Molecular Cloud

1982 ◽  
pp. 385-389
Author(s):  
Julian H. Krolik ◽  
Timothy R. Kallman
Keyword(s):  
Molecular Cloud ◽  
X Ray

X-ray ionization and the Orion molecular cloud

1983 ◽  
Vol 267 ◽  
pp. 610 ◽  
Author(s):  
J. H. Krolik ◽  
T. R. Kallman
Keyword(s):  
Molecular Cloud ◽  
X Ray

The Distance to an X-Ray Shadowing Molecular Cloud in Ursa Major

1996 ◽  
Vol 464 ◽  
pp. 836 ◽  
Author(s):  
Robert A. Benjamin ◽  
Kim A. Venn ◽  
Daniel D. Hiltgen ◽  
Christopher Sneden
Keyword(s):  
Molecular Cloud ◽  
X Ray

The X-ray shadow of the high-latitude molecular cloud MBM 12

1993 ◽  
Vol 409 ◽  
pp. L21 ◽  
Author(s):  
S. L. Snowden ◽  
D. McCammon ◽  
F. Verter
Keyword(s):  
High Latitude ◽  
Molecular Cloud ◽  
X Ray

The Origin of X-Ray Emission from a Galactic Center Molecular Cloud: Low-Energy Cosmic-Ray Electrons

2002 ◽  
Vol 568 (2) ◽  
pp. L121-L125 ◽  
Author(s):  
F. Yusef-Zadeh ◽  
C. Law ◽  
M. Wardle
Keyword(s):  
Molecular Cloud ◽  
Galactic Center ◽  
Cosmic Ray ◽  
Low Energy ◽  
X Ray

scholarly journals High Resolution X-ray Images of Puppis a and IC 443

1983 ◽  
Vol 101 ◽  
pp. 289-293
Author(s):  
R. Petre ◽  
C. R. Canizares ◽  
P. F. Winkler ◽  
F. D. Seward ◽  
R. Willingale ◽  
...  
Keyword(s):  
High Resolution ◽  
Interstellar Medium ◽  
Molecular Cloud ◽  
Supernova Remnants ◽  
Surface Brightness ◽  
Middle Aged ◽  
X Ray ◽  
Giant Molecular Cloud

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.

scholarly journals Interaction of the SS433 Jet with the Interstellar Medium

2000 ◽  
Vol 195 ◽  
pp. 419-420
Author(s):  
P. O'Neill ◽  
R. Sood ◽  
P. Durouchoux ◽  
S. Safi-Harb
Keyword(s):  
Interstellar Medium ◽  
Molecular Cloud ◽  
Surrounding Medium ◽  
Strong Association ◽  
X Ray

X-ray emission observed from the SS433/W50 system has been interpreted as resulting from the interaction of the binary jets with the surrounding medium. We have been carrying out millimetre wavelength measurements of this system. We find no evidence for the association of a molecular cloud with the eastern jet, but we do find evidence for a strong association with the western jet.

Deep Near‐Infrared Observations of the X‐Ray–emitting Class 0 Protostar Candidates in the Orion Molecular Cloud 3

2002 ◽  
Vol 573 (1) ◽  
pp. 270-274 ◽  
Author(s):  
Masahiro Tsujimoto ◽  
Katsuji Koyama ◽  
Yohko Tsuboi ◽  
George Chartas ◽  
Miwa Goto ◽  
...  
Keyword(s):  
Molecular Cloud ◽  
Near Infrared ◽  
Infrared Observations ◽  
X Ray

scholarly journals Spectral properties of X-ray bright variable sources in the Taurus molecular cloud

2006 ◽  
Vol 468 (2) ◽  
pp. 485-499 ◽  
Author(s):  
E. Franciosini ◽  
I. Pillitteri ◽  
B. Stelzer ◽  
G. Micela ◽  
K. R. Briggs ◽  
...  
Keyword(s):  
Molecular Cloud ◽  
Spectral Properties ◽  
X Ray ◽  
Taurus Molecular Cloud

scholarly journals THeoretical Thermal X-Ray Maps of Supernova Remnants in Non-Uniform Media

1983 ◽  
Vol 101 ◽  
pp. 393-397 ◽  
Author(s):  
H. W. Yorke ◽  
G. Tenorio-Tagle ◽  
P. Bodenheimer
Keyword(s):  
Axial Symmetry ◽  
Molecular Cloud ◽  
Supernova Remnants ◽  
Supernova Remnant ◽  
X Ray ◽  
Cooling Effects

The evolution of a supernova remnant resulting from an explosion near the edge of a molecular cloud is calculated with a 2-D hydrodynamical code (axial symmetry assumed). Cooling effects have been included. 1 kev X-ray maps of the remnant at different evolutionary times and different viewing angles are presented.

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