Results 31 to 40 of about 2,487,342 (212)
Accretion of mass onto a white dwarf (WD) in a binary system can lead to stellar explosions. If a WD accretes from stellar wind of a distant evolved giant in a symbiotic binary, it can undergo occasional outbursts in which it brightens by several ...
Augustin Skopal
doaj +1 more source
The helium-rich cataclysmic variable SBSS 1108+574 [PDF]
We present time-resolved spectroscopy and photometry of the dwarf nova SBSS 1108+574, obtained during the 2012 outburst. Its quiescent spectrum is unusually rich in helium, showing broad, double-peaked emission lines from the accretion disc. We measure a
Koff, R.A. +36 more
core +2 more sources
Exploring the application of new telescope technologies in the testing of dwarf novae accretion models [PDF]
Includes abstract.Includes bibliographical references (p. 261-273.)In this thesis I investigate emerging telescope technologies and demonstrate, within the context of accretion in cataclysmic variables (CVs), their role in contributing to the stellar ...
Spark, Mellony
core +1 more source
Pole-On Cataclysmic Variables as Be Stars [PDF]
Cataclysmic-variable stars (CVs) are technically Be stars, since Balmer emission lines appear in their spectra. In general, CV spectra are so unusual that they are easily recognized. The main features are extremely broad, shallow hydrogen lines with broad, faint emission cores.
openaire +1 more source
The properties of cataclysmic variables in photometric H alpha surveys [PDF]
We report on the properties of 71 known cataclysmic variables (CVs) in photometric H alpha emission-line surveys. Our study is motivated by the fact that the Isaac Newton Telescope (INT) Photometric H alpha Survey of the northern galactic plane (IPHAS ...
Rodriguez-Flores, E.R. +19 more
core +1 more source
Irradiation of the secondary star in cataclysmic variables [PDF]
It is shown how the relative strength of the Na I doublet over the surface of the secondary star can be calculated from radial velocity curves obtained using the Na I absorption feature around 8190 A. The results for 11 dwarf novae and one magnetic cataclysmic binary system are presented.
S. Davey, R. C. Smith
openaire +1 more source
Cataclysmic variable stars are semi-detached binary systems consisting of a white dwarf primary star and a late-type secondary star. The secondary star in these systems is over- filling its Roche lobe, which enables a mass transfer to occur between the ...
Kára, Jan
core +1 more source
Hubble space telescope STIS spectroscopy of the peculiar nova-like variables BK Lyn, V751 Cygni, and V380 Oph [PDF]
We obtained Hubble STIS spectra of three nova-like variables: V751 Cygni, V380 Oph, and—the only confirmed nova-like variable known to be below the period gap—BK Lyn.
Gänsicke, B. T. (Boris T.) +6 more
core +1 more source
White Dwarfs in Cataclysmic Variable Stars: Surface Temperatures and Evolution [PDF]
A summary is presented of what is currently known about the surface temperatures of accreting white dwarfs (WDs) detected in non-magnetic and magnetic cataclysmic variables (CVs) based upon synthetic spectral analyses of far ultraviolet data.
Edward M. Sion
doaj +1 more source
By in situ reaction blending, DOPO‐HQ and THEIC were added to PLA with MDI to construct a phosphorus containing polyurethane network, which significantly improved the flame retardant and anti‐dripping properties of polylactic acid composites. ABSTRACT Polylactic acid (PLA) is highly flammable and prone to severe melt dripping during combustion, which ...
Chiyuan Chen +4 more
wiley +1 more source

