Continued Timing and Monitoring of New and Old Rotating Radio Transients

Details Continued Timing and Monitoring of New and Old Rotating Radio Transients Continued Timing and Monitoring of New and Old Rotating Radio Transients

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atnf.prop.1833m&link_type=abstract

ATNF proposal P511, Semester: October, 2008

Other

Galactic, Parkes

Scientific paper

We request continuing timing and monitoring observations of 13 rotating radio transients. These sources are rotating neutron stars which are detectable only through their sporadic radio bursts. The observations proposed here are crucial for understanding the emission mechanism of these sources and for determining how they relate to other neutron star populations. we also aim to maintain the phase-connected timing solutions achieved during the last observing semester to determine positions, ages and magnetic fields. These observations are the cornerstone of an extensive campaign at X-ray, radio and infrared wavelengths.

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