Results 211 to 220 of about 14,394 (262)

Precise Tailoring 3D Printed In Situ Toughening Low-k Microwave Transparent Structure via Thiol-acrylate Chain Transfer Behavior. [PDF]

Adv Sci (Weinh)
Bian C, Zheng K, Chen R, Gu W, Zhong G, Liang D, Deng L, Chu H.   +7 more
europepmc   +1 more source

Exploring human-induced flood risks and sustainable urban resilience in Iwo Nigeria with focus on awareness drivers and mitigation pathways. [PDF]

Sci Rep
Ogunbode TO, Opabunmi BA, Adeyi ST, Akinwale EA, Ayodele IM.   +4 more
europepmc   +1 more source

Plant diversity induces shifts from microbial generalists to specialist by enhancing niche differentiation, microbiome connectivity, and network stability in a temperate grassland. [PDF]

Environ Microbiome
Finck J, Chowdhury S, Griffiths RI, Malik AA, Eisenhauer N, Lange M, Mendes LW, Gleixner G.   +7 more
europepmc   +1 more source

Leucine Aminopeptidase to Spleen Length Ratio: A Novel Noninvasive Model for Predicting Esophageal Gastric Variceal Bleeding in Patients With Liver Cirrhosis. [PDF]

Gastroenterol Res Pract
Zhu C, Jiang Y, Liu Y, Bian Z, Luo L.
europepmc   +1 more source

Port-site metastases after diagnostic laparoscopy in advanced ovarian cancer: a case report and a systematic review of the literature. [PDF]

Front Surg
De Tommasi O, Bigardi S, Incognito GG, Modena L, Goretti C, Spagnol G, Ettore C, Ettore G, Noventa M, Saccardi C, Tozzi R.   +10 more
europepmc   +1 more source

PSD3 en PSR

, 2023
openaire   +1 more source

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Pairs of pulsars (PSR) and the origin of PSR

Astrophysics and Space Science, 1986
The results of research on pairs of PSR which were possibly components of disrupted binaries, seem to advance further arguments in favour of the idea, suggested by some authors, that most of PSR were formed in binary systems.
Massimo Fracassini, Paola Maggi, Laura E. Pasinetti   +2 more
openaire   +1 more source

Decametric Pulse Radioemission from PSR 0809, PSR 1133, and PSR 1919

Nature Physical Science, 1973
RECEPTION of decametric radiation from pulsars is extremely hindered by deterioration of the signal-to-noise ratio in this band caused by a decrease in the pulsar's bandwidth and the high values of the background temperature. Nevertheless, the existing observational results at 38 MHz (ref. 1) and 40 MHz (ref.
YU. M. BRUCK, B. YU. USTIMENKO
openaire   +1 more source

Are PSR 0656+14, PSR 0950+08, and PSR 1822-09 gamma-ray pulsars?

Astrophysics and Space Science, 1993
The possible discovery of three new gamma-ray pulsars PSR 0656+14, PSR 0950+08, and PSR 1822-09 (Ma, Lu, Yu, and Young, 1993) in data obtained with the COS-B experiment is reinvestigated using a refined technique for pulsar light curve analysis. The results of this study do not confirm the previously claimed gamma-ray pulsar nature of any of these ...
Lawrence E. Brown, Dieter H. Hartmann
openaire   +1 more source