Results 291 to 300 of about 562,012 (337)
Rsp5/NEDD4 and ESCRT regulate TDP-43 toxicity and turnover via an endolysosomal clearance mechanism. [PDF]
J Cell BiolByrd A +6 more
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Successful Resolution of Coronary Thrombus in a Child With Kawasaki Disease and Giant Coronary Artery Aneurysms Using Anticoagulation Therapy. [PDF]
CureusAlmasaeid H, Saleh AA, Obaidy H.
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Pulmonary Sarcomatoid (Pleomorphic) Carcinoma Presenting As Secondary Spontaneous Pneumothorax in Diffuse Cystic Lung Disease: A Case Report. [PDF]
CureusAnnan GK +4 more
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Nocardia farcinica Brain Abscess in a Glucocorticoid-Treated Patient with Giant-Cell Arteritis: A Case Report. [PDF]
Am J Case RepValenti S +4 more
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Comprehensive treatment and surgical features of giant hepatic hemangioma with Kasabach-Merritt syndrome in an adult. [PDF]
Hepatobiliary Surg NutrDeng Y +8 more
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2021
In 2012, we published a paper in the Journal of Critical Globalization Studies titled 'Imperialism and Financialism: The Story of a Nexus'. Our topic was the chameleon-like Marxist notion of imperialism and how its different theories related to finance.
Bichler, Shimshon, Nitzan, Jonathan
openaire +1 more source
In 2012, we published a paper in the Journal of Critical Globalization Studies titled 'Imperialism and Financialism: The Story of a Nexus'. Our topic was the chameleon-like Marxist notion of imperialism and how its different theories related to finance.
Bichler, Shimshon, Nitzan, Jonathan
openaire +1 more source
Scientific American, 2007
This article reports that astronomers have found an exoplanet that likely survived the red giant phase of its parent star. Named V391 Pegasi, it belongs to a class of subdwarf stars that flicker. Researchers noticed the regularity of the flickering and says it is a planet at least 3 times bigger than Jupiter.
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This article reports that astronomers have found an exoplanet that likely survived the red giant phase of its parent star. Named V391 Pegasi, it belongs to a class of subdwarf stars that flicker. Researchers noticed the regularity of the flickering and says it is a planet at least 3 times bigger than Jupiter.
openaire +1 more source
EAS Publications Series, 2015
A new rotation model for post-main sequence stars is proposed. This model quantitatively reproduces core and surface rotation rates of subgiant stars, as well as the core rotation of helium-burning clump stars.
Y. Kissin, C. Thompson
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A new rotation model for post-main sequence stars is proposed. This model quantitatively reproduces core and surface rotation rates of subgiant stars, as well as the core rotation of helium-burning clump stars.
Y. Kissin, C. Thompson
openaire +1 more source