Observations of the galactic radio structure CTB 63 (G47.5 + 6.0)

Details Observations of the galactic radio structure CTB 63 (G47.5 + 6.0) Observations of the galactic radio structure CTB 63 (G47.5 + 6.0)

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989aj.....97.1721c&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 97, June 1989, p. 1721-1726.

Astronomy and Astrophysics

Astronomy

2

Extragalactic Radio Sources, Galactic Radio Waves, Galactic Structure, Supernova Remnants, Astronomical Spectroscopy, Brightness Temperature, High Resolution, Radio Galaxies

Scientific paper

The radio source CTB 63 is extended and diffuse and has been regarded as a possible galactic supernova remnant. New observations at 408 and 1420 MHz, made with the DRAO synthesis telescope, delineate the boundary and suggest that it is a galactic spur rather than a discrete supernova remnant. The spur has a length of about 6 deg and at one extremity merges with the diffuse galactic disk emission; it is clearly nonthermal. Small-diameter sources in the region, most of which are extragalactic background sources, are also cataloged.

Affiliated with

Also associated with

No associations

Rating

Observations of the galactic radio structure CTB 63 (G47.5 + 6.0) 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 Observations of the galactic radio structure CTB 63 (G47.5 + 6.0), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observations of the galactic radio structure CTB 63 (G47.5 + 6.0) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1849747