Radio emission from X-ray sources

Details Radio emission from X-ray sources Radio emission from X-ray sources

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..68..509a&link_type=abstract

Astrophysics and Space Science, vol. 68, no. 2, Apr. 1980, p. 509-511.

Astronomy and Astrophysics

Astronomy

Galactic Radiation, Plasma Oscillations, Radio Emission, Radio Sources (Astronomy), X Ray Sources, Binary Stars, Lagrange Coordinates, Neutron Stars, Stellar Mass Accretion

Scientific paper

Point X-ray sources with faint variable radio sources are investigated. It is suggested that the radio emission from point X-ray sources is due to plasma oscillations in the outer region of an accretion disk around a neutron star in a binary system where the inflow of matter through the inner Lagrange point impinges on the disk. A possible test of the suggestion would be to observe the radio sources at wavelengths much longer than 2 cm. The absence of radio emission at low frequencies would support the proposed model.

Affiliated with

Also associated with

No associations

Rating

Radio emission from X-ray sources 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 Radio emission from X-ray sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio emission from X-ray sources will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1697550