Results 31 to 40 of about 152,722 (200)

Self-Similar Solution of Hot Accretion Flow with Anisotropic Pressure

open access: yesUniverse, 2019
For the accretion flow in extremely low-luminosity active galactic nuclei, such as our Galactic center (Sgr A*) and M 87, the collisional mean-free path of ions may be much larger than its gyroradius.
De-Fu Bu, Pei-Yao Xu, Bo-Cheng Zhu
doaj   +1 more source

Evolution of Interstellar Medium, Star Formation, and Accretion at High Redshift [PDF]

open access: yes, 2017
ALMA observations of the long wavelength dust continuum are used to estimate the interstellar medium (ISM) masses in a sample of 708 galaxies at z = 0.3 to 4.5 in the COSMOS field.
N. Scoville   +23 more
semanticscholar   +1 more source

Magellan Adaptive Optics Imaging of PDS 70: Measuring the Mass Accretion Rate of a Young Giant Planet within a Gapped Disk [PDF]

open access: yesAstrophysical Journal Letters, 2018
PDS 70b is a recently discovered and directly imaged exoplanet within the wide (≳40 au) cavity around PDS 70. Ongoing accretion onto the central star suggests that accretion onto PDS 70b may also be ongoing.
K. Wagner   +13 more
semanticscholar   +1 more source

Hot Accretion Flow in Two-Dimensional Spherical Coordinates: Considering Pressure Anisotropy and Magnetic Field

open access: yesUniverse, 2019
For systems with extremely low accretion rate, such as Galactic Center Sgr A* and M87 galaxy, the ion collisional mean free path can be considerably larger than its Larmor radius. In this case, the gas pressure is anisotropic to magnetic field lines.
Hui-Hong Deng, De-Fu Bu
doaj   +1 more source

A Long-Term Study of Ultraluminous X-ray Sources in NGC 891

open access: yesUniverse, 2021
We perform empirical fits to the Chandra and XMM-Newton spectra of three ultraluminous X-ray sources (ULXs) in the edge-on spiral galaxy NGC 891, monitoring the region over a 17-year time window.
Nicholas M. Earley    +2 more
doaj   +1 more source

Super-Eddington Accretion Disks around Supermassive Black Holes [PDF]

open access: yesAstrophysical Journal, 2017
We use global three-dimensional radiation magnetohydrodynamical simulations to study accretion disks onto a black hole with accretion rates varying from to . We initialize the disks with a weakly magnetized torus centered at either 50 or 80 gravitational
Yan-Fei 飞 Jiang 姜 燕   +2 more
semanticscholar   +1 more source

Acclimatization Drives Differences in Reef-Building Coral Calcification Rates

open access: yesDiversity, 2020
Coral reefs are susceptible to climate change, anthropogenic influence, and environmental stressors. However, corals in Kāneʻohe Bay, Hawaiʻi have repeatedly shown resilience and acclimatization to anthropogenically-induced rising temperatures and ...
Kelsey Archer Barnhill   +6 more
doaj   +1 more source

Whole Body Nutrient Accretion, Growth Performance and Total Tract Nutrient Retention Responses of Broilers to Supplementation of Xylanase and Phytase Individually or in Combination in Wheat-Soybean Meal Based Diets

open access: yesThe Journal of Poultry Science, 2008
Growth performance, total tract nutrient retention and whole body nutrient accretion rates responses of broilers to supplementation of enzymes containing phytase or xylanase activities were investigated using 300 broilers.
Oluyinka A. Olukosi, Olayiwola Adeola
doaj   +1 more source

Growth of asteroids, planetary embryos, and Kuiper belt objects by chondrule accretion [PDF]

open access: yesScience Advances, 2015
Chondrules, tiny spheres found in primitive meteorites, accumulate through gas drag to form asteroids and planetary embryos. Chondrules are millimeter-sized spherules that dominate primitive meteorites (chondrites) originating from the asteroid belt. The
A. Johansen   +3 more
semanticscholar   +1 more source

Plate-tectonic metallogeny Ural-Timan-Paleoasian segment of the Eurasia on the base of mobilistic reconstructions

open access: yesЛитосфера, 2017
General positions on plate-tectonic metallogeny are presented and the grounds for singling out the metallogenic factors of orogenic systems are given. Mobilistic paradigma corresponds to the genotype of orogens and belts which being formed at the expense
Viktor M. Necheukhin, Elena N. Volchek
doaj   +1 more source

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