activity
19982005
most citedThe Highly Relativistic Binary Pulsar PSR J0737-3039A: Discovery and Implications

3 citations · 16 across the 16 of their papers we have counts for

collaborators
Showing astro-phShow all

20 papers · 1 filter

astro-ph20051 cited

Pulsar Astrometry at the Microarcsecond Level

W. H. T. Vlemmings, S. Chatterjee, W. F. Brisken +12

Determination of pulsar parallaxes and proper motions addresses fundamental astrophysical questions. We have recently finished a VLBI astrometry project to determine the proper mot…

astro-ph20042 cited

Fundamental Physics with the SKA:Strong-Field Tests of Gravity Using Pulsars and Black Holes

M. Kramer

The Square-Kilometre-Array (SKA) will be a radio telescope with a collecting area that will exceed that of existing telescopes by a factor of a hundred or so. This contribution sum…

astro-ph20043 cited

The Highly Relativistic Binary Pulsar PSR J0737-3039A: Discovery and Implications

M. Burgay, N. D'Amico, A. Possenti +10

PSR J0737-3039A is a millisecond pulsar with a spin period of 22.7 ms included in a double-neutron star system with an orbital period of 2.4 hrs. Its companion has also been detect…

astro-ph20042 cited

Two clocks in the PSR J0737--3039 binary system and their implications for the system's origin and evolution

D. R. Lorimer, M. Burgay, P. C. C. Freire +8

As discussed elsewhere in these proceedings, the double pulsar system is a magnificent laboratory for gravitational physics and for studying pulsar magnetospheres. Here we consider…

astro-ph2003

Observational manifestations of young neutron stars: Spin-powered pulsars

Michael Kramer

The largest number of known young neutron stars are observed as spin-powered pulsars. While the majority of those are detected at radio frequencies, an increasing number can be stu…

astro-ph20032 cited

Giant pulses in Millisecond Pulsars

B. C. Joshi, M. Kramer, A. G. Lyne +2

Giant pulses (GPs), occasional individual pulses with an intensity 100 times the average intensity, have been detected in four pulsars todate. Their origin is not well understood,…