Results 121 to 130 of about 270 (168)
Binarity and Accretion in AGB Stars: HST/STIS Observations of UV Flickering in Y Gem. [PDF]
Sahai R +5 more
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Atomic diffusion and mixing in old stars - VIII. Chemical abundance variations in the globular cluster M4 (NGC 6121). [PDF]
Nordlander T +3 more
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Commodity risk assessment of <i>Vitis</i> spp. plants from Moldova. [PDF]
EFSA Panel on Plant Health (PLH) +37 more
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NOVAE VERSUS DWARF NOVAE - ENERGY-SOURCES AND SYSTEMATICS
MALLAMA, AD, TRIMBLE, VL
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Syntaxonomical Remarks on the Garrigues from Apulia (S Italy) and Neighboring Territories. [PDF]
Tomaselli V +8 more
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Commodity risk assessment of maple veneer sheets from Canada. [PDF]
EFSA Panel on Plant Health (PLH) +29 more
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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
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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
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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).
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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).
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The decay of dwarf nova outbursts
Space Science Reviews, 1985Simultaneous 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
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