Radio and X-Ray Emission Associated with the Supernova Remnant G352.7-0.1

Details Radio and X-Ray Emission Associated with the Supernova Remnant G352.7-0.1 Radio and X-Ray Emission Associated with the Supernova Remnant G352.7-0.1

2005-11-16

arxiv.org/abs/astro-ph/0511477v1

Astronomy and Astrophysics

Astrophysics

2 pages, 2 figures. To appear in the proceedings of "The X-Ray Universe 2005" conference, 2005 Sept 26-30, El Escorial, Madrid

Scientific paper

We report on new VLA radio and XMM-Newton X-ray observations of the SNR G352.7-0.1. These high sensitivity, high resolution data reveal that G352.7-0.1 belongs to the thermal composite morphological class. Small scale structures in radio and X-ray emission are not always correlated and are different for the different X-rays bands examined. The distance to G352.7-0.1 can be constrained between 6.6 and 8.4 kpc. The study of the HI suggests that G352.7-0.1 is located within a cavity probably created by the stellar wind of the precursor star.

Affiliated with

Also associated with

No associations

Rating

Radio and X-Ray Emission Associated with the Supernova Remnant G352.7-0.1 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Radio and X-Ray Emission Associated with the Supernova Remnant G352.7-0.1, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio and X-Ray Emission Associated with the Supernova Remnant G352.7-0.1 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-580747