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20032009
most citedDetection of a Hot Subdwarf Companion to the Be Star FY Canis Majoris

77 citations · 484 across the 14 of their papers we have counts for

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astro-ph20084 cited

The Full Spectrum Galactic Terrarium: MHz to TeV Observations of Various Critters

Mallory S. E. Roberts, C. Brogan, S. Ransom +13

Multi-wavelength studies at radio, infrared, optical, X-ray, and TeV wavelengths have discovered probable counterparts to many Galactic sources of GeV emission detected by EGRET. T…

astro-ph200817 cited

Detection of Magnetic Massive Stars in the Open Cluster NGC 3766

M. Virginia McSwain

A growing number of observations indicate that magnetic fields are present among a small fraction of massive O- and B-type stars, yet the origin of these fields remains unclear. He…

astro-ph200877 cited

Detection of a Hot Subdwarf Companion to the Be Star FY Canis Majoris

Geraldine J. Peters, Douglas R. Gies, Erika D. Grundstrom +1

The rapid rotation of Be stars may be caused in some cases by past mass and angular momentum accretion in an interacting binary in which the mass donor is currently viewed as a sma…

astro-ph200829 cited

New Massive Binaries in the Cygnus OB2 Association

Daniel C. Kiminki, M. Virgina McSwain, Henry A. Kobulnicky

As part of an ongoing study to determine the distribution of orbital parameters for massive binaries in the Cygnus OB2 Association, we present the orbital solutions for two new sin…

astro-ph200818 cited

Dynamical Masses for the Large Magellanic Cloud Massive Binary System [L72] LH 54-425

S. J. Williams, D. R. Gies, T. J. Henry +8

We present results from an optical spectroscopic investigation of the massive binary system [L72] LH~54-425 in the LH 54 OB association in the Large Magellanic Cloud. We revise the…

astro-ph200872 cited

Stellar Wind Variations During the X-ray High and Low States of Cygnus X-1

D. R. Gies, C. T. Bolton, R. M. Blake +10

We present results from Hubble Space Telescope UV spectroscopy of the massive X-ray binary system, HD226868 = Cyg X-1. The spectra were obtained at both orbital conjunction phases…