K
K. W. Weiler
Researcher at United States Naval Research Laboratory
Publications - 96
Citations - 1522
K. W. Weiler is an academic researcher from United States Naval Research Laboratory. The author has contributed to research in topics: Supernova & Radio astronomy. The author has an hindex of 22, co-authored 96 publications receiving 1478 citations. Previous affiliations of K. W. Weiler include NASA Lunar Science Institute.
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The Long Wavelength Array
Namir E. Kassim,Emil Polisensky,Tracy E. Clarke,Brian C. Hicks,P. C. Crane,K. P. Stewart,Paul S. Ray,K. W. Weiler,L. J. Rickard,T. J. W. Lazio,W. M. Lane,A. S. Cohen,Michael E. Nord,W. C. Erickson,Richard A. Perley +14 more
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X-ray, Optical, and Radio Observations of the Type II Supernovae 1999em and 1998S
David Pooley,Walter H. G. Lewin,D. W. Fox,Jon M. Miller,Christina K. Lacey,S. D. Van Dyk,K. W. Weiler,Richard A. Sramek,Alexei V. Filippenko,Douglas C. Leonard,Stefan Immler,Roger A. Chevalier,A. C. Fabian,Claes Fransson,K. Nomoto +14 more
TL;DR: In this article, Chandra X-ray data indicate non-radiative interaction of SN ejecta with a power-law density profile (rho \propto r^{-n} with n ~ 7) with a pre-SN wind with a low mass-loss rate of ~2 \times 10-6} M_sun/yr for a wind velocity of 10 km/sec, in agreement with radio mass loss rate estimates.
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Deceleration in the Expansion of SN1993J
J. M. Marcaide,Antonio Alberdi,Eduardo Ros,P. J. Diamond,Irwin I. Shapiro,J. C. Guirado,D. L. Jones,F. Mantovani,Miguel A. Pérez-Torres,Robert A. Preston,R. T. Schilizzi,Richard A. Sramek,Corrado Trigilio,S. D. Van Dyk,K. W. Weiler,Alan R. Whitney +15 more
TL;DR: In this paper, the authors measured the deceleration of supernova ejecta and circumstellar material in standard supernova explosion models using VLBI observations at wavelengths of 3.6 and 6 cm in the period 6 to 42 months after explosion.
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Radio emission from a type I supernova : SN 1983.51 in NGC 5236.
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A Decade of SN 1993J: Discovery of Radio Wavelength Effects in the Expansion Rate
J. M. Marcaide,Ivan Marti-Vidal,Ivan Marti-Vidal,Antonio Alberdi,Miguel A. Pérez-Torres,Eduardo Ros,Eduardo Ros,Philip J. Diamond,J. C. Guirado,L. Lara,Irwin I. Shapiro,Chris Stockdale,K. W. Weiler,F. Mantovani,Robert A. Preston,R. T. Schilizzi,Richard A. Sramek,Corrado Trigilio,S. D. Van Dyk,Alan R. Whitney +19 more
TL;DR: In this article, the authors studied the growth of the shell-like radio structure of supernova SN 1993J in M 81 from September 1993 to October 2003 with very-long-baseline interferometry (VLBI) observations at the wavelengths of 3.6, 6, and 18 cm.