activity
20052009
most citedA Radio Pulsar/X-ray Binary Link

591 citations · 630 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2009591 cited

A Radio Pulsar/X-ray Binary Link

Anne M. Archibald, Ingrid H. Stairs, Scott M. Ransom +15

Radio pulsars with millisecond spin periods are thought to have been spun up by transfer of matter and angular momentum from a low-mass companion star during an X-ray-emitting phas…

astro-ph200721 cited

The Kinematic Evolution of Strong MgII Absorbers

Andrew C. Mshar, Jane C. Charlton, Ryan S. Lynch +2

We consider the evolution of strong (W_r(2796) > 0.3A) MgII absorbers, most of which are closely related to luminous galaxies. Using 20 high resolution quasar spectra from the VLT/…

astro-ph200718 cited

Physical Properties of Weak MgII Absorbers at z~2

Ryan S. Lynch, Jane C. Charlton

We present the results of photoionization modeling of nine weak MgII (W_r<0.3 Ang) quasar absorption line systems with redshifts 1.4<z<2.4 obtained with the Ultraviolet and Visual…

astro-ph2005

The Nature of Weak MgII Absorbing Structures

Nikola Milutinovic, Jane R. Rigby, Joseph R. Masiero +3

We consider geometries and possible physical models for weak low ionization absorbers based on the relative incidence of low and high ionization absorption systems. We found a tota…

astro-ph2005

A survey of weak MgII absorbers at redshift <z>=1.78

Ryan S. Lynch, Jane C. Charlton, Tae-Sun Kim

The exact nature of weak MgII absorbers (those with W_r(2796) < 0.3 A) is a matter of debate, but most are likely related to areas of local star formation or supernovae activity ou…

astro-ph2005

A Survey of Analogs to Weak MgII Absorbers in the Present

Anand Narayanan, Jane C. Charlton, Joe R. Masiero +1

We present the results of a survey of the analogs of weak MgII absorbers (rest frame equivalent width W(2796) < 0.3 A) at 0 < z < 0.3. Our sample consisted of 25 HST/STIS echelle q…