activity
20042015
most citedA Long Look at the Be/X-Ray Binaries of the Small Magellanic Cloud

89 citations · 606 across the 24 of their papers we have counts for

collaborators

23 papers

astro-ph.EP2015★ 24 cited

The Need for Speed in Near-Earth Asteroid Characterization

J. L. Galache, C. L. Beeson, K. K. McLeod +1

We have used Minor Planet Center data and tools to explore the discovery circumstances and properties of the currently known population of over 10,000 NEAs, and to quantify the cha…

astro-ph.EP2013★ 2 cited

Alternate Science Investigations for the Kepler Spacecraft: Precision Rotation Periods and Shapes of Near-Earth Asteroids

Martin Elvis, José Luis Galache, Gareth V. Williams

We propose to use a modest fraction of the re-purposed Kepler mission time and apertures to greatly increase the quantity and quality of our knowledge of near-Earth asteroids (NEAs…

astro-ph.HE2012★ 9 cited

Chandra Observations of the Collisional Ring Galaxy NGC 922

A. H. Prestwich, J. L. Galache. T. Linden, V. Kalogara +5

In this paper we report on Chandra observations of the starburst galaxy NGC 922. NGC 922 is a drop-through ring galaxy with an expanding ring of star formation, similar in many res…

astro-ph.HE2012★ 13 cited

A period distribution of X-ray binaries observed in the central region of M31 with Chandra and HST

R. Barnard, J. L. Galache, M. Garcia +4

Almost all Galactic black hole binaries with low mass donor stars are transient X-ray sources; we expect most of the X-ray transients observed in external galaxies to be black hole…

astro-ph.HE2009★ 10 cited

Be/X-ray binary SXP6.85 undergoes large Type II outburst in the Small Magellanic Cloud

L. J. Townsend, M. J. Coe, V. A. McBride +6

The Small Magellanic Cloud (SMC) Be/X-ray binary pulsar SXP6.85 = XTE J0103-728 underwent a large Type II outburst beginning on 2008 August 10. The source was consistently seen for…

astro-ph.HE2009★ 41 cited

X-ray and Radio Variability of M31*, The Andromeda Galaxy Nuclear Supermassive Black Hole

Michael R. Garcia, Richard Hextall, Frederick K. Baganoff +6

We confirm our earlier tentative detection of M31* in X-rays and measure its light-curve and spectrum. Observations in 2004-2005 find M31* rather quiescent in the X-ray and radio.…