arXiv · astro-ph/0603258
A tale of two populations: Rotating Radio Transients and X-ray Dim Isolated Neutron Stars
Abstract
We highlight similarities between recently discovered Rotating Radio Transients and X-ray Dim Isolated Neutron Stars. In particular, it is shown that X-ray Dim Isolated Neutron Stars have a birthrate comparable to that of Rotating Radio Transients. On the contrary, magnetars have too low a formation rate to account for the bulk of the radio transient population. The consequences of the recent detection of a thermal X-ray source associated with one of the Rotating Radio Transients on the proposed scenarios for these sources are also discussed.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
S. B. Popov, R. Turolla, A. Possenti. 2006-03-10. A tale of two populations: Rotating Radio Transients and X-ray Dim Isolated Neutron Stars. https://doi.org/10.1111/j.1745-3933.2006.00166.x
Cite the original work for its findings. Save a collection to share your selection of sources.