Results 201 to 210 of about 3,875 (235)
Prior evidence suggested inconsistent findings in terms of the relationship between obesity and inflammatory bowel disease (IBD) occurrence. We demonstrated that both general and central obesities were associated with an increased risk of developing IBD, ulcerative colitis, and Crohn's disease in a large‐scale prospective cohort.
Qian Zhang +5 more
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ABSTRACT Background A significant complication of pediatric tonsillectomy is post‐tonsillectomy bleeding (PTB). Management within and outside of the operating room (OR) is not standardized. We consolidated international similarities and differences in PTB management.
Gina M. Spencer +8 more
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ABSTRACT The insulating core is an important part of pillar composite insulators used in power transmission systems. Traditional insulating core materials suffer from various problems that can threaten the reliability of insulated equipment. Syntactic foam (SF) exhibits excellent properties, such as a low density, water penetration resistance and high ...
Le Li +8 more
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Our study demonstrates how life history trade‐offs and pair bonds influence winter roosting in red kites. Analysing long‐term GPS data from 216 individuals, we reveal marked behavioural plasticity in communal roosting: young, non‐breeding males are most likely to join communal roosts, whereas breeding pairs predominantly roost together near their ...
Benedetta Catitti +6 more
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Demographic buffering in natural populations: A multi‐level perspective
We introduce a multi‐level framework that unites stochastic elasticities with nonlinear selection to test demographic buffering. Applying it across mammals reveals a key insight: ecological robustness to variability often decouples from evolutionary constraint, reshaping how we understand resilience under environmental stochasticity.
Gabriel Silva Santos +4 more
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Fronting in Old Catalan: Asymmetries between Narration and Reported Speech1
Abstract This article explores the distribution, syntax, and information structure of XVS clauses in the narrative text and the reported speech of a thirteenth‐century Old Catalan chronicle, the Llibre dels Fets. It is shown that XVS occurs mainly within reported speech and in embedded clauses.
Afra Pujol i Campeny
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Nature, 1946
ON-February 10 the variable star T Coronae Borealis, normally of magnitude 9, was seen to have blazed up to magnitude 3. This star had a typical nova outburst in 1866, when it was the first nova to be examined spectroscopically. Unlike other novae, its spectrum after fading was of late type with strong absorption bands of titanium oxide.
F. J. M. STRATTON, H. E. BUTLER
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ON-February 10 the variable star T Coronae Borealis, normally of magnitude 9, was seen to have blazed up to magnitude 3. This star had a typical nova outburst in 1866, when it was the first nova to be examined spectroscopically. Unlike other novae, its spectrum after fading was of late type with strong absorption bands of titanium oxide.
F. J. M. STRATTON, H. E. BUTLER
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The Recurrent Novae and Their Relation with Classical Novae
AIP Conference Proceedings, 2002Recurrent novae (RNe) are a subclass of cataclysmic variables classified based on recorded observations of more than one nova outburst. They form a small, but heterogeneous group of objects, with 10 known members, that undergo classical nova‐like outbursts, with the significant differences being in the amplitude and the frequency of the outbursts.
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Studies of Classical and Recurrent Novae
Publications of the Astronomical Society of the Pacific, 1992Novae belong to the cataclysmic-variable class of objects. These objects are interacting binary star systems consisting of a Roche-lobe filling secondary, on or near the main sequence, losing hydrogen-rich material through the inner-Lagrangian point onto an accretion disk that surrounds the primary, which, in most cases, is a white dwarf.
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The Evolutionary Significance of Recurrent Novae
International Astronomical Union Colloquium, 1979Within the past few years, it has become increasingly apparent that common novae and dwarf novae must owe their origin to binary systems of much larger initial separation than they now have (Paczynski 1976; Ritter 1975, 1976; Webbink 1975). This was demanded by the realization that the white dwarfs in these binaries are generally quite massive (see for
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