A possible turn-over in pulsar spectra at mm-wavelengths?

Details A possible turn-over in pulsar spectra at mm-wavelengths? A possible turn-over in pulsar spectra at mm-wavelengths?

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995yera.conf...16k&link_type=abstract

The XXVIIth Young European Radio Astronomers Conference, ed. D.A. Green and W. Steffen, in association with Cambridge University

Astronomy and Astrophysics

Astronomy

Scientific paper

We present the results of recent pulsar observations at frequencies
between 27.9 GHz and 34.8 GHz, i.e. in a wavelength range of 10.75 mm to
8.61 mm, made with the Effelsberg radiotelescope. The measured flux
densities of two out of nine detected pulsars suggest that the spectrum
flattens at high frequencies or even shows a turn-over.

Affiliated with

Also associated with

No associations

Rating

A possible turn-over in pulsar spectra at mm-wavelengths? 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 possible turn-over in pulsar spectra at mm-wavelengths?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A possible turn-over in pulsar spectra at mm-wavelengths? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-852929