14 citations · 29 across the 4 of their papers we have counts for
4 papers
Using Shell Models to Investigate Clumping in the WN4 Star HD 50896
Brian L. Flores, D. John Hillier, Luc Dessart
The spectra of Wolf-Rayet (WR) stars exhibit strong, broad emission lines that originate in the wind. These winds are radiatively driven and are susceptible to hydrodynamic instabi…
Using Shell Models to Investigate Clumping in the Wind of the O7Iaf+ Supergiant AzV83
Brian L. Flores, D. John Hillier
Hot massive stars exhibit strong stellar winds that enrich the surrounding interstellar medium and affect the stars' evolution. However, the winds are inhomogeneous (clumped) and a…
Effects of Strong Photospheric Dissipation on the Spectra and Structure of Accretion Disks with Non-zero Inner Torque
Theodore Dezen, Noah Egger, Lwendo Mwansa
We present numerical calculations of spectra and structure of accretion disks models appropriate for near-Eddington luminosity black hole X-ray binaries (BHB). Our work incorporate…
Spectra and Structure of Accretion Disks with Nonzero Inner Torque
Theodore Dezen, Bryan Flores
We present numerical spectral and vertical structure calculations appropriate for near-Eddington-luminosity, radiation-pressure-dominated accretion disks around stellar-mass black…