most citedExtrasolar Carbon Planets

49 citations

6 papers

astro-ph200549 cited

Extrasolar Carbon Planets

Marc J. Kuchner, S. Seager

We suggest that some extrasolar planets <~ 60 Earth masses will form substantially from silicon carbide and other carbon compounds. Pulsar planets and low-mass white dwarf planets…

astro-ph20041 cited

Magnetised plasma turbulence in clusters of galaxies

A. A. Schekochihin, S. C. Cowley, R. M. Kulsrud +2

Cluster plasmas are magnetised already at very low magnetic field strength. Low collisionality implies that conservation of the first adiabatic invariant results in an anisotropic…

astro-ph2004

GBT Observations of Very Low Mass Binary Millisecond Pulsars: A Search for Eclipses

David J. Nice, Ingrid H. Stairs, Zaven Arzoumanian

We searched for eclipses of two millisecond pulsars, PSR J1807-2459 and PSR B1908+00. These pulsars are in very low mass binary systems with orbital parameters similar to those of…

astro-ph20043 cited

Arecibo Measurements of Pulsar--White Dwarf Binaries: Evidence for Heavy Neutron Stars

David J. Nice, Eric M. Splaver, Ingrid H. Stairs

We summarize constraints on neutron star masses from ongoing timing observations of pulsar-white dwarf binaries at Arecibo. The trend is toward pulsar masses larger than the canoni…

astro-ph2004

The Power of Exploratory Chandra Observations

S. C. Gallagher, G. T. Richards, W. N. Brandt +1

With its excellent spatial resolution, low background, and hard-band response, the Chandra X-ray Observatory is ideal for performing exploratory surveys. These efficient, sensitive…

astro-ph2004

The repeating microlensing event OGLE-2003-BLG-095: A plausible case for microlensing of a binary source

Matthew J. Collinge

The apparently repeating microlensing event OGLE-2003-BLG-095 is analyzed. Data were obtained from the OGLE Internet archive and exist in the public domain. The source is relativel…