741 citations · 8.2k across the 109 of their papers we have counts for
63 papers · 1 filter
Modeling UX Ursae Majoris: An abundance of challenges
Albert P. Linnell, Patrick Godon, Ivan Hubeny +2
We present a system model for optical and far UV spectra of the nova-like variable UX UMa involving a white dwarf, secondary star, gas stream, hot spot and accretion disk using our…
Spectrum and atmosphere models of irradiated transiting extrasolar giant planets
Ivan Hubeny, Adam Burrows
We show that a consistent fit to observed secondary eclipse data for several strongly irradiated transiting planets demands a temperature inversion (stratosphere) at altitude. Such…
Optical Albedo Theory of Strongly-Irradiated Giant Planets: The Case of HD 209458b
A. Burrows, L. Ibgui, I. Hubeny
We calculate a new suite of albedo models for close-in extrasolar giant planets and compare with the recent stringent upper limit for HD 209458b of Rowe et al. using MOST. We find…
A Far Ultraviolet Archival Study of Cataclysmic Variables: I. FUSE and HST/STIS Spectra of the Exposed White Dwarf in Dwarf Nova Systems
P. Godon, E. M. Sion, P. E. Barrett +3
We present a synthetic spectral analysis of Far Ultraviolet Spectroscopic Explorer (FUSE) and Hubble Space Telescope/Space Telescope Imaging Spectrograph (HST/STIS) spectra of 5 dw…
Hubble Space Telescope STIS Spectroscopy of Long Period Dwarf Novae in Quiescence
E. M. Sion, B. T. Gaensicke, K. S. Long +5
We present the results of a synthetic spectral analysis of HST STIS spectra of five long period dwarf novae obtained during their quiescence to determine the properties of their wh…
Synthetic Spectrum Constraints on a Model of the Cataclysmic Variable QU Carinae
Albert P. Linnell, Patrick Godon, Ivan Hubeny +3
Neither standard model SEDs nor truncated standard model SEDs fit observed spectra of QU Carinae with acceptable accuracy over the range 900Åto 3000Å. Non-standard model SEDs fit t…