MULTI-WAVELENGTH ANALYSIS OF THE GALACTIC SUPERNOVA REMNANT MSH 11-61A
Due to its centrally bright X-ray morphology and limb brightened radio profile, MSH 11-61A (G290.1-0.8) is classified as a mixed morphology supernova remnant (SNR). H i and CO observations determined that the SNR is interacting with molecular clouds found toward the north and southwest regions of th...
Main Authors: | Auchettl, Katie (Author), Slane, Patrick (Author), Castro, Daniel (Contributor), Foster, Adam R. (Author), Smith, Randall K. (Author) |
---|---|
Other Authors: | MIT Kavli Institute for Astrophysics and Space Research (Contributor) |
Format: | Article |
Language: | English |
Published: |
IOP Publishing,
2015-11-13T13:37:16Z.
|
Subjects: | |
Online Access: | Get fulltext |
Similar Items
-
A radiocontinuum study of the supernova remnant MSH 11-61A
by: Filipović M.D., et al.
Published: (2005-01-01) -
FERMI -LAT OBSERVATIONS OF SUPERNOVA REMNANTS KESTEVEN 79
by: Auchettl, Katie, et al.
Published: (2015) -
HIGH-ENERGY EMISSION FROM THE COMPOSITE SUPERNOVA REMNANT MSH 15-56
by: Temim, Tea, et al.
Published: (2015) -
UNRAVELING THE ORIGIN OF OVERIONIZED PLASMA IN THE GALACTIC SUPERNOVA REMNANT W49B
by: Lopez, Laura A., et al.
Published: (2015) -
Multi-Wavelength View of Supernova Remnants
by: Manami Sasaki
Published: (2014-12-01)