Is the G18.95-1.1 radio source a shell-type supernova remnant with a central object?

Details Is the G18.95-1.1 radio source a shell-type supernova remnant with a central object? Is the G18.95-1.1 radio source a shell-type supernova remnant with a central object?

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988natur.332..136p&link_type=abstract

Nature (ISSN 0028-0836), vol. 332, March 10, 1988, p. 136, 137.

Astronomy and Astrophysics

Astronomy

8

Radio Sources (Astronomy), Supernova Remnants, Astronomical Spectroscopy, Light Emission, Nonthermal Radiation, Radiant Flux Density, Radio Telescopes, X Rays

Scientific paper

Fürst et al. (1985) have reported that the nonthermal galactic radio source G18.95-1.1 shows arc-like structures pointing towards the radio peak near its centre, and that its morphology does not conform to any known class of supernova remnants. They propose an accreting binary origin for the source. In view of the suggested peculiar morphology of G18.95-1.1, high-resolution (96×36 arc s) low-frequency (327 MHz) observations were made using the Ooty Synthesis Radio Telescope. This high-resolution map of G18.95-1.1 is consistent with the conventional shell-type morphology around a central object.

Affiliated with

Also associated with

No associations

Rating

Is the G18.95-1.1 radio source a shell-type supernova remnant with a central object? 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 Is the G18.95-1.1 radio source a shell-type supernova remnant with a central object?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Is the G18.95-1.1 radio source a shell-type supernova remnant with a central object? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1691753