Year: 2008
Type: conference-paper
Abstract: Rotating RAdio Transients are a new class of neutron stars discovered through the emission of radio bursts. Eleven sources are known up to now, but population studies predict these objects to be more numerous than the normal radio pulsar population. Multiwavelength observations of these peculiar objects are in progress to disentangle their spectral energy distribution, and then study in detail their nature. In this review I will report on the current state of the art on these objects.
Source: AIP conference proceedings
DOI: 10.1063/1.2840387
Authors: Nanda Rea, Maura McLaughlin, Ye-Fei Yuan, Xiang-Dong Li, Dong Lai
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W1586419052
