Characterizing the standardization properties of type ia supernovae in the z band with hierarchical Bayesian modelling
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Erin E Hayes↗
SEARCH · Engineering Papers
Results for “Supernovae”
Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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Comparisons of Type Ia Supernova Light Curves in the UV and Optical with the Swift Ultra-violet/Optical Telescope
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Yaswant Devarakonda↗
The Twins Embedding of Type Ia Supernovae. I. The Diversity of Spectra at Maximum Light
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K. Boone↗
A Galactic dust devil: far-infrared observations of the Tornado supernova remnant candidate
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H Chawner↗
SN 2022jli: A Type Ic Supernova with Periodic Modulation of Its Light Curve and an Unusually Long Rise
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T. Moore↗
Pre-supernova evolution - Neutrino stars.
Stellar evolution for high temperature, predominantly neutrino processes, noting breakdown of homology relation between density and temperature
NEUTRINO↗
Neutrino processes and pair formation in massive stars and supernovae
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Fowler, W. A.↗
Supernovae, neutrinos, and neutron stars.
Photodisintegration of iron into helium and neutrino annihilation process cause hydrostatic and dynamic instabilities that produce star collapse
Chiu, H.-Y.↗
On Supernova Hydrodynamics
Rebuttal to Colgate criticism of Arnett investigation of gravitational collapse of nonrotating massive stars, discussing energy transport, equation of state and neutrino effects
Arnett, W. D.↗
The approach to supernova implosion conditions.
Conditions for neutrino emission processes domination of highly evolved star luminosity, disputing Fowler-Hoyle collapse temperature for 30 solar mass stars
Chiu, H. Y.↗
A search for energetic gamma-ray emission from the supernova remnant Cassiopeia A.
Energetic gamma rays emission from radio source Cassiopeia A by high altitude balloon observations, using high resolution telescope
May, T. C.↗
Supernovae studied with a ground level atmospheric fluorescence
A monitoring experiment was undertaken late 1968 to search for photon bursts of extraterrestrial origin. The experiment and the results of the observations to date are summarized. The method of detection employs ground-based photomultiplier tubes which are sensitive to the secondary fluorescence light that would be produced when the primary pulse is absorbed in the atmosphere.
Bertsch, D. L.↗
Observational evidence against supernovae being the source of the universal X-ray background.
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Mack, J. E.↗
Surface brightness measurements of supernova remanants in the energy band 0.15 - 4 keV and an XUV survey from an altitude controlled rocket
Reports are presented concerning the flight of Aerobee 170, 13.063 UG. The papers presented include: soft X-rays for Cygnus X-1 and Cygnus X-2; X-ray spectrum of the entire Cygnus loop; X-ray surface brightness of the Cygnus loop; and observations of He II 304 A and He I 584 a nightglow.
Garmire, G. P.↗
Photometry of supernova 1972 in NGC 5253.
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Lee, T. A.↗
Spectrophotometry of the supernova in NGC 5253 from 0.33 to 2.2 microns.
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Kirshner, R. P.↗
X-ray observations of the supernova remnant IC 443
Presented observation data from OSO-7 are shown to confirm the identification of IC 443 as an X-ray source, with a spectrum which is consistent with either thermal bremsstrahlung or a power law. These data lead to an age of 3400 years for IC 443, much younger than previous estimates.
Winkler, P. F., Jr.↗
Limit on X-ray emission from a supernova during maximum light
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Sprott, G. F.↗