Zobrazeno 1 - 10
of 20
pro vyhledávání: '"Adam Burr"'
Publikováno v:
Otolaryngologic Clinics of North America. 56:305-312
Autor:
Mattison J. Flakus, Sean P. Kent, Eric M. Wallat, Antonia E. Wuschner, Erica Tennant, Poonam Yadav, Adam Burr, Menggang Yu, Gary E Christensen, Joseph M. Reinhardt, John E. Bayouth, Andrew M. Baschnagel
Publikováno v:
Radiotherapy and Oncology. 182:109553
Publikováno v:
Radiation oncology journal.
Purpose: Optimal radiotherapy treatment volumes for patients with locally advanced hypopharynx squamous cell carcinoma should ensure maximal tumor coverage with minimal inclusion of normal surrounding structures. Here we evaluated the effectiveness o
Autor:
Dan Milisavljevic, Tea Temim, Ilse De Looze, Danielle Dickinson, J. Martin Laming, Robert Fesen, John C. Raymond, Richard G. Arendt, Jacco Vink, Bettina Posselt, George G. Pavlov, Ori D. Fox, Ethan Pinarski, Bhagya Subrayan, Judy Schmidt, William P. Blair, Armin Rest, Daniel Patnaude, Bon-Chul Koo, Jeonghee Rho, Salvatore Orlando, Hans-Thomas Janka, Moira Andrews, Michael J. Barlow, Adam Burrows, Roger Chevalier, Geoffrey Clayton, Claes Fransson, Christopher Fryer, Haley L. Gomez, Florian Kirchschlager, Jae-Joon Lee, Mikako Matsuura, Maria Niculescu-Duvaz, Justin D. R. Pierel, Paul P. Plucinsky, Felix D. Priestley, Aravind P. Ravi, Nina S. Sartorio, Franziska Schmidt, Melissa Shahbandeh, Patrick Slane, Nathan Smith, Niharika Sravan, Kathryn Weil, Roger Wesson, J. Craig Wheeler
Publikováno v:
The Astrophysical Journal Letters, Vol 965, Iss 2, p L27 (2024)
We present initial results from a James Webb Space Telescope (JWST) survey of the youngest Galactic core-collapse supernova remnant, Cassiopeia A (Cas A), made up of NIRCam and MIRI imaging mosaics that map emission from the main shell, interior, and
Externí odkaz:
https://doaj.org/article/e2737691eb9b4fc79f78fcc284ecfa83
Publikováno v:
The Astrophysical Journal Letters, Vol 964, Iss 1, p L16 (2024)
In this paper, we derive correlations between core-collapse supernova observables and progenitor core structures that emerge from our suite of 20 state-of-the-art 3D core-collapse supernova simulations carried to late times. This is the largest such
Externí odkaz:
https://doaj.org/article/8cd9fc860e8841cda7f98b4bf1096195
Publikováno v:
The Astrophysical Journal, Vol 975, Iss 1, p 12 (2024)
In this paper, we calculate the energy, signal-to-noise ratio (SNR), detection range, and angular anisotropy of the matter, matter memory, and neutrino memory gravitational-wave (GW) signatures of 21 three-dimensional initially nonrotating core-colla
Externí odkaz:
https://doaj.org/article/05bd44237f2e4c50aea103605b5c2128
Autor:
Tianshu Wang, Adam Burrows
Publikováno v:
The Astrophysical Journal, Vol 974, Iss 1, p 39 (2024)
We report nucleosynthetic results for both ^44 Ti and nickel isotopes for 18 three-dimensional (3D) core-collapse supernova (CCSN) simulations extended to ∼20 s after bounce. We find that many of our long-term models are able to achieve ^44 Ti/ ^56
Externí odkaz:
https://doaj.org/article/d01cfcc2421344dfb6a60a16852abde4
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 274, Iss 2, p 34 (2024)
The equation of state of hydrogen–helium (H–He) mixtures plays a vital role in the evolution and structure of gas giant planets and exoplanets. Recent equations of state that account for H–He interactions, coupled with H–He immiscibility curv
Externí odkaz:
https://doaj.org/article/8eea32f78fd648a6838c58221374e064
Publikováno v:
The Astrophysical Journal, Vol 971, Iss 1, p 104 (2024)
We introduce APPLE , a novel planetary evolution code designed specifically for the study of giant exoplanet and Jovian planet evolution in the era of Galileo, Juno, and Cassini. With APPLE , state-of-the-art equations of state for hydrogen, helium,
Externí odkaz:
https://doaj.org/article/6d9ccd600569448b9bcb322748df48d9
Autor:
Tianshu Wang, Adam Burrows
Publikováno v:
The Astrophysical Journal, Vol 969, Iss 2, p 74 (2024)
We here focus on the behavior of supernovae that technically explode in 1D (spherical symmetry). When simulated in 3D, however, the outcomes of representative progenitors of this class are quite different in almost all relevant quantities. In 3D, the
Externí odkaz:
https://doaj.org/article/37d30303b44744d09cef0fe596c90206