Results 31 to 40 of about 8,370 (124)

The effect of orbital damping during planet migration on the Inclination and Eccentricity Distributions of Neptune Trojans [PDF]

open access: yes, 2016
We explore planetary migration scenarios for formation of high inclination Neptune Trojans (NTs) and how they are affected by the planetary migration of Neptune and Uranus. If Neptune and Uranus's eccentricity and inclination were damped during planetary migration, then their eccentricities and inclinations were higher prior and during migration than ...
arxiv   +1 more source

The Intrinsic Neptune Trojan Orbit Distribution: Implications for the Primordial Disk and Planet Migration [PDF]

open access: yes, 2014
The present-day orbit distribution of the Neptune Trojans is a powerful probe of the dynamical environment of the outer solar system during the late stages of planet migration. In this work, I conservatively debias the inclination, eccentricity, and libration amplitude distributions of the Neptune Trojans by reducing a priori unknown discovery and ...
arxiv   +1 more source

Duration of Hospitalization in Association with Type of Inhalation Therapy Used in the Management of Children with Nonsevere, Acute Bronchiolitis

open access: yesPediatrics and Neonatology, 2016
Acute bronchiolitis is one of the main respiratory emergencies in young children. Although supportive therapy is recommended, substantial inconsistency in the clinical usage of inhaled treatments has been reported.
Jamie M. Pinto   +2 more
doaj   +1 more source

Neptune's wild days: constraints from the eccentricity distribution of the classical Kuiper Belt [PDF]

open access: yes, 2012
Neptune's dynamical history shaped the current orbits of Kuiper belt objects (KBOs), leaving clues to the planet's orbital evolution. In the "classical" region, a population of dynamically "hot" high-inclination KBOs overlies a flat "cold" population with distinct physical properties.
arxiv   +1 more source

Jumping Neptune Can Explain the Kuiper Belt Kernel [PDF]

open access: yes, 2015
The Kuiper belt is a population of icy bodies beyond the orbit of Neptune. A particularly puzzling and up-to-now unexplained feature of the Kuiper belt is the so-called `kernel', a concentration of orbits with semimajor axes a~44 AU, eccentricities e~0.05, and inclinations i<5 deg.
arxiv   +1 more source

Origin and Dynamical Evolution of Neptune Trojans - I: Formation and Planetary Migration [PDF]

open access: yesMon.Not.Roy.Astron.Soc.398: 1715-1729,2009, 2009
We present the results of detailed dynamical simulations of the effect of the migration of the four giant planets on both the transport of pre-formed Neptune Trojans, and the capture of new Trojans from a trans-Neptunian disk. We find that scenarios involving the slow migration of Neptune over a large distance (50Myr to migrate from 18.1AU to its ...
arxiv   +1 more source

Meningitis from invasive Streptococcus agalactiae in a healthy young adult

open access: yesIDCases, 2020
Streptococcus agalactiae is well known to be a potential etiology of bacterial meningitis in neonates. Invasive S. agalactiae has been also reported in nonpregnant adults.
Asseel Al-Bayati   +7 more
doaj  

Assessing the contribution of Centaur impacts to ice giant luminosities [PDF]

open access: yes, 2015
Voyager 2 observations revealed that the internal luminosity of Neptune is an order of magnitude higher than that of Uranus. If the two planets have similar interior structures and cooling histories, the luminosity of Neptune can only be explained by invoking some energy source beyond gravitational contraction.
arxiv   +1 more source

A multidisciplinary approach: Case report of an abdominal aortic aneurysm with type IIIA endoleak in the setting of cholangitis

open access: yesSAGE Open Medical Case Reports, 2023
Endoleaks are a common complication of endovascular aortic aneurysm repair and often lead to aneurysm rupture. We report a complex case of a Type IIIA endoleak in a patient with suspected cholangitis.
Emmanuel Ihionkhan   +4 more
doaj   +1 more source

Compositional diversity in the atmospheres of hot Neptunes, with application to GJ 436b [PDF]

open access: yesAstrophys. J., 777, 34 (2013), 2013
Neptune-sized extrasolar planets that orbit relatively close to their host stars -- often called "hot Neptunes" -- are common within the known population of exoplanets and planetary candidates. Similar to our own Uranus and Neptune, inefficient accretion of nebular gas is expected produce hot Neptunes whose masses are dominated by elements heavier than
arxiv   +1 more source

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