Radio and X-ray properties of galactic supernova remnants G7.7-3.7 and G344.7-0.1

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

1

X-Ray Sources (Astronomical), Stellar Atmospheres, Interstellar Matter, Astronomical Telescopes, X-Ray Sources, X-Ray Bursts, Stellar Atmospheres, Radiative Transfer, Opacity And Line Formation, Interstellar Dust Grains, Diffuse Emission, Infrared Cirrus, X- And Gamma-Ray Telescopes And Instrumentation

Scientific paper

We report on new radio and X-ray observations of two galactic SNRs: G7.7-3.7 and G344.7-0.1. The high resolution, high sensitivity radio data show several new structures in both remnants. In the X-ray regime, the XMM-Newton data for G7.7-3.7 reveal the existence of thermal soft X-ray emission coinciding with the radio southern limb of the remnant, and a point-like feature with a spectrum suggestive of a compact X-ray source or a PWN. In the case of G344.7-0.1, the new XMM-Newton image shows clumpy features and diffuse emission filling the interior of the remnant. The X-ray spectral investigation inferres enhanced abundances which imply the presence of SN ejecta in this SNR.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Radio and X-ray properties of galactic supernova remnants G7.7-3.7 and G344.7-0.1 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 properties of galactic supernova remnants G7.7-3.7 and G344.7-0.1, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio and X-ray properties of galactic supernova remnants G7.7-3.7 and G344.7-0.1 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1644180

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.