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Uncovering the orbital dynamics of stars hidden inside their powerful winds: application to Carinae and RMC 140
David Grant, Katherine Blundell, James Matthews
Determining accurate orbits of binary stars with powerful winds is challenging. The dense outflows increase the effective photospheric radius, precluding direct observation of the…
Disc wind models for FU Ori objects
Kelly Milliner, James H. Matthews, Knox S. Long +1
We present disc wind models aimed at reproducing the main features of the strong Na I resonance line P-Cygni profiles in the rapidly-accreting pre-main sequence FU Ori objects. We…
The Impact of Accretion Disk Winds on the Optical Spectra of Cataclysmic Variables
James H. Matthews, Christian Knigge, Knox S. Long +2
Many high-state non-magnetic cataclysmic variables (CVs) exhibit blue-shifted absorption or P-Cygni profiles associated with ultraviolet (UV) resonance lines. These features imply…