An Imaging and Spectroscopic Study of the Supernova Remnant RCW 103 (G332.4-0.4) with the CHANDRA X-ray Observatory
The explosion of a massive star results in an immense expulsion of energy and stellar debris (ejecta) that are heated to extremely high temperatures forming what is known as a super va remnant (SNR). Presented is a CHANDRA 0.5-10 keV X-ray study of the SNR RCW 103, a bright SNR that contains the unu...
Main Author: | Braun, Chelsea |
---|---|
Other Authors: | Safi-Harb, Samar (Physics and Astronomy) |
Published: |
2016
|
Subjects: | |
Online Access: | http://hdl.handle.net/1993/31185 |
Similar Items
-
OB Stars Near the Supernova Remnant RCW 86
by: Westerlund, B. E.
Published: (1969) -
PROBING X-RAY ABSORPTION AND OPTICAL EXTINCTION IN THE INTERSTELLAR MEDIUM USING CHANDRA OBSERVATIONS OF SUPERNOVA REMNANTS
by: Foight, Dillon R., et al.
Published: (2016) -
Observational data on Galactic supernova remnants: II. The supernova remnants within l = 90°-270°
by: Guseinov O.H., et al.
Published: (2004-01-01) -
Observational data on galactic supernova remnants: I. The supernova remnants within l = 0◦ - 90◦
by: Guseinov O.H., et al.
Published: (2003-01-01) -
Observational data on Galactic supernova remnants III: The supernova remnants within l = 270°-360°
by: Guseinov O.H., et al.
Published: (2004-01-01)