A metre-wave outburst from the QSO 1055 + 018

Details A metre-wave outburst from the QSO 1055 + 018 A metre-wave outburst from the QSO 1055 + 018

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.209..215s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 209, July 1, 1984, p. 215-226.

Other

11

Brightness Temperature, Quasars, Very High Frequencies, Astronomical Coordinates, Astronomical Maps, Long Term Effects, Radiant Flux Density

Scientific paper

Observations of the QSO 1055 + 018 with the Culgoora circular array show that the source flux density doubled at 160 MHz and tripled at 80 MHz during the first seven months of 1983, while complementary observations between 0.843 and 15 GHz revealed no significant changes. Since the 80-MHz quiescent brightness temperature probably exceeds the inverse Compton limit of about 10 to the 12th K for incoherent synchrotron emission, the extreme-brightness temperatures deduced from the time variability at meter wavelengths may naturally be explained by the brightening of a coherent source. Slow interstellar scintillations provide another possible explanation.

Affiliated with

Also associated with

No associations

Rating

A metre-wave outburst from the QSO 1055 + 018 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 A metre-wave outburst from the QSO 1055 + 018, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A metre-wave outburst from the QSO 1055 + 018 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1707939