Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986aj.....91..343d&link_type=abstract
Astronomical Journal (ISSN 0004-6256), vol. 91, Feb. 1986, p. 343-353.
Astronomy and Astrophysics
Astronomy
11
Continuous Spectra, Hydrogen, Interstellar Matter, Radio Astronomy, Supernova Remnants, Astronomical Maps, Centimeter Waves, Density Distribution, Hydrogen Clouds
Scientific paper
1410 MHz radio continuum and H I 21 cm line observations have been performed on an extended area that contains the SNR G296.5+10.0. Two additional radio-continuum sources have been identified in the 1410 MHz map, namely (1) G300.1+9.4, which is classified as a faint SNR, located at a distance comparable to that of G296.5+10.0, and (2) G300.8+11.7, with a broken spectrum and a possible double structure unresolvable with the present resolution. The observations reproduce the theoretically expected outcome of two interacting supernova remnants. In addition, some small H I clouds accelerated to relatively high velocities are observed to be positionally coincident with the SNRs.
Colomb Fernando R.
Dubner Gloria M.
Giacani Elsa B.
No associations
LandOfFree
1410 MHz continuum and H I line observations towards the SNR G296.5 + 10.0 and nearby sources - Evidences of two SNRs tunneling through the interstellar medium 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 1410 MHz continuum and H I line observations towards the SNR G296.5 + 10.0 and nearby sources - Evidences of two SNRs tunneling through the interstellar medium, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and 1410 MHz continuum and H I line observations towards the SNR G296.5 + 10.0 and nearby sources - Evidences of two SNRs tunneling through the interstellar medium will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1674158