Results 71 to 80 of about 352 (180)
Molecular Oncology, Volume 20, Issue S1, Page 1-692, August 2026.Abstracts submitted to the ‘EACR 2026 Congress: Innovative Cancer Science’, from 08–11 June 2026 and accepted by the Congress Organising Committee are published in this Supplement of Molecular Oncology, an affiliated journal of the European Association for Cancer Research (EACR).
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Environmental Microbiology Reports, Volume 18, Issue 3, June 2026.The polyphasic approach (morphology, physiology, biochemistry and genetics) was used to characterize Acetobacter indonesiensis strain UNPADCC 01‐5, which was isolated from oncom merah. The strain's potential as a culture for acidic fermentations and a biofunctional agent was supported by its adaptive characteristics, which included acid tolerance ...
Yolani Syaputri +9 more
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The Astrophysical JournalGamma-ray bursts (GRBs), both from the merger of binary compact objects (short GRBs) and the collapse of massive stars (long GRBs), are expected to occur in dense environments, e.g., the accretion disks of active galactic nuclei (AGNs).
Hao-Yu Yuan, Wei-Hua Lei
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Starving Accretion Disks in the Center of Galaxies: the Examples of Sgr A* and M31
, 1994 The low accretion rate inferred for the GC source Sgr A* requires a distinct type of accretion disk -- a starving disk. We investigate the structure of this type of disk within the framework of thin Keplerian disk models taking into account relativistic effects, detailed opacitiy tables and turbulent heat transport.
Falcke, H., Heinrich, O. M.
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Radiative Cooling and Viscous Dissipation in Molecular Accretion Disks at the Nuclei of Galaxies
The Astrophysical Journal, 1998 Key processes are examined in the heating and cooling of molecular gas with emphasis on environments for water masers at the nuclei of galaxies. The exchange of infrared radiation between the gas and dust grains is evaluated in determining the cooling of the gas and in determining the thermal coupling between the gas and the dust grains.
S. J. Desch, B. K. Wallin, W. D. Watson
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The Astrophysical JournalMagnetically arrested disks (MADs) have attracted much attention in recent years. The formation of MADs is usually attributed to the accumulation of a sufficient amount of dynamically significant poloidal magnetic flux.
Jia-Wen Li, Xinwu Cao
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Gas Evolution in Disk Galaxies : Disk Stability, Gas Accretion & The Impacts of Spiral Density Waves [PDF]
, 2010 Diese Arbeit untersucht viele Aspekte der zeitlichen Entwicklung von Gas in Scheibengalaxien. Eine einfache und effektive Methode zur Initialisierung einer dreidimensionalen Gasscheibe in detailliertem Gleichgewicht wurde entwickelt. Mithilfe dieser Methode untersuchen wir theoretische Vorhersagen über Stabilität und 'Swing' Verstärkung ...
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Insights from Analytical Theory of Eccentric Circumbinary Disks
The Astrophysical JournalEccentric cavities in circumbinary disks precess on timescales much longer than the binary orbital period. These long-lived steady states can be understood as trapped modes in an effective potential primarily determined by the binary quadrupole and the ...
Marcela Grcić +2 more
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Disk Assembly of the Milky Way Suggested from the Time-resolved Chemical Abundance
The Astrophysical JournalBoth simulations and observations suggest that the disk assembly of galaxies is governed by the interplay between coplanar gas inflow, ex-planar gas outflow, and in situ star formation on the disk, known as the leaky accretion disk.
Enci Wang +3 more
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Shock Waves in the Magnetic Reconnection in the Flares on the Accretion Disk of the Sgr A*
The Astrophysical JournalSgr A* often shows bright, episodic flares observationally, but the mechanism of the flares' intermittent brightening is not very clear. Many people believe the flares may be formed by the nonthermal particles, which can be a consequence of the magnetic ...
Tian-Le Zhao +3 more
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