Radio upper limits for the accreting millisecond X-ray pulsar IGR J17511-3057

Details Radio upper limits for the accreting millisecond X-ray pulsar IGR J17511-3057 Radio upper limits for the accreting millisecond X-ray pulsar IGR J17511-3057

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2232....1m&link_type=abstract

The Astronomer's Telegram, #2232

Astronomy and Astrophysics

Astronomy

4

Radio, Binaries, Neutron Stars, Pulsars, Transients

Scientific paper

We report on recent radio observations of the newly-detected accreting millisecond X-ray pulsar, IGR J17511-3057 (ATels #2196, #2197, #2198, #2199, #2215, #2216, #2220, #2221). We used the Very Large Array (VLA) to observe the source under observing program AM971. The array was in its relatively compact 'C' and 'DNC' configurations, and the observations were made at 8.46 GHz. In no case was the source significantly detected.

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