The Massive Binary Pulsar J1740-3052

A. G. Lyne; F. Camilo (Columbia); I. H. Stairs (UBC); M. Kramer (JBO); N. D'Amico (Bologna); R. N. Manchester (ATNF); V. M. Kaspi (McGill)

arxiv: astro-ph/0211004 · v1 · submitted 2002-11-01 · 🌌 astro-ph

The Massive Binary Pulsar J1740-3052

I. H. Stairs (UBC) , R. N. Manchester (ATNF) , A. G. Lyne , M. Kramer (JBO) , V. M. Kaspi (McGill) , F. Camilo (Columbia) , N. D'Amico (Bologna) This is my paper

classification 🌌 astro-ph

keywords companionj1740-3052pulsarbinarydiscussimplicationsleastmasses

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The young pulsar J1740-3052 is in an 8-month orbit with a companion of at least 11 solar masses. We present multifrequency GBT and Parkes timing observations, and discuss implications for the nature of the companion.

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The Massive Binary Pulsar J1740-3052

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