Results 121 to 130 of about 270 (168)

Binarity and Accretion in AGB Stars: HST/STIS Observations of UV Flickering in Y Gem. [PDF]

open access: yesAstrophys J, 2018
Sahai R   +5 more
europepmc   +1 more source

Commodity risk assessment of <i>Vitis</i> spp. plants from Moldova. [PDF]

open access: yesEFSA J
EFSA Panel on Plant Health (PLH)   +37 more
europepmc   +1 more source

Syntaxonomical Remarks on the Garrigues from Apulia (S Italy) and Neighboring Territories. [PDF]

open access: yesPlants (Basel)
Tomaselli V   +8 more
europepmc   +1 more source

Commodity risk assessment of maple veneer sheets from Canada. [PDF]

open access: yesEFSA J
EFSA Panel on Plant Health (PLH)   +29 more
europepmc   +1 more source

The dwarf nova dippers

Advances in Space Research, 1988
Previous papers have shown that the dwarf nova OY Car has an extensive vertical disk structure during its superoutbursts. This structure is analogous to that seen in the low mass X-ray binaries (LMXBs), in that the whole disk flares toward its edge, and there is a bulge or 'dark spot' where the mass transfer stream meets the disk edge.
T. Naylor   +3 more
openaire   +1 more source

Dwarf-Nova Outbursts

Publications of the Astronomical Society of the Pacific, 1996
Outburst mechanisms of dwarf novae are discussed. There is a rich variety in outburst behaviors of non-magnetic cataclysmic variable stars, starting from non-outbursting nova-like stars to various sub-classes of dwarf novae (i.e., U Gem-type, Z Cam-type, and SU UMa-type).
openaire   +1 more source

The decay of dwarf nova outbursts

Space Science Reviews, 1985
Simultaneous observations at different wavelengths of the decay of dwarf-nova outbursts, show an earlier return to the quiescence level at shorter wavelengths. These observations, which show completely new aspects of outbursts, can provide strong tests for outburst models and accretion-disc theory.
H. van der Woerd, J. Heise
openaire   +1 more source

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