High time resolution observations of CU Virginis

Details High time resolution observations of CU Virginis High time resolution observations of CU Virginis

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atnf.prop.3100h&link_type=abstract

ATNF proposal P741, Semester: April, 2010

Physics

Magnetic Fields, Transients, Parkes

Scientific paper

CU Virginis is the prototypical example of a new class of stellar radio transient. This star provides a unique laboratory for studying coherent radio emission mechanisms in a stellar environment. Observations taken for this proposal will allow us to determine whether the pulses are formed out a continuous emission process or discrete flares and thereby constrain the emission mechanism.

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