SILICON CARBIDE GRAINS OF TYPE C PROVIDE EVIDENCE FOR THE PRODUCTION OF THE UNSTABLE ISOTOPE 32Si IN SUPERNOVAE (English)
- New search for: Pignatari, M.
- New search for: Pignatari, M.
- New search for: Zinner, E.
- New search for: Bertolli, M. G.
- New search for: Trappitsch, R.
- New search for: Hoppe, P.
- New search for: Rauscher, T.
- New search for: Fryer, C.
- New search for: Herwig, F.
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In:
The astrophysical journal / 2
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771
, 1
; L7
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2013
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ISSN:
- Article (Journal) / Print
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Title:SILICON CARBIDE GRAINS OF TYPE C PROVIDE EVIDENCE FOR THE PRODUCTION OF THE UNSTABLE ISOTOPE 32Si IN SUPERNOVAE
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Contributors:Pignatari, M. ( author ) / Zinner, E. / Bertolli, M. G. / Trappitsch, R. / Hoppe, P. / Rauscher, T. / Fryer, C. / Herwig, F. / Hirschi, R. / Timmes, F. X.
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Published in:The astrophysical journal / 2 ; 771, 1 ; L7
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Publisher:
- New search for: Institute of Physics Publ.
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Place of publication:London
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Publication date:2013
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ISSN:
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ZDBID:
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Type of media:Article (Journal)
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Type of material:Print
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Language:English
- New search for: 39.22
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Keywords:
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Classification:
BKL: 39.22 Astrophysik -
Source:
Table of contents – Volume 771, Issue 1
The tables of contents are generated automatically and are based on the data records of the individual contributions available in the index of the TIB portal. The display of the Tables of Contents may therefore be incomplete.
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DETECTION OF THE AMMONIUM ION IN SPACEThis work was based on observations carried out with the IRAM 30 m telescope. IRAM is supported by INSU/CNRS (France), MPG (Germany), and IGN (Spain)Cernicharo, J. et al. | 2013
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GAMMA-RAY BLAZARS NEAR EQUIPARTITION AND THE ORIGIN OF THE GeV SPECTRAL BREAK IN 3C 454.3Cerruti, Matteo et al. | 2013
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SILICON CARBIDE GRAINS OF TYPE C PROVIDE EVIDENCE FOR THE PRODUCTION OF THE UNSTABLE ISOTOPE 32Si IN SUPERNOVAEPignatari, M. et al. | 2013
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DISCOVERY OF AN ULTRAMASSIVE PULSATING WHITE DWARFHermes, J. J. et al. | 2013
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MAIN-BELT COMET P/2012 T1 (PANSTARRS)Some of the data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration, and made possible by the generous financial support of the W. M. Keck Foundation, the Magellan Telescopes located at Las Campanas Observatory, Chile, and the Southern Astrophysical Research (SOAR) telescope, which is a joint project of the Ministério da Ciência, Tecnologia, e Inovação (MCTI) da República Federativa do Brasil, the U.S. National Optical Astronomy Observatory (NOAO), the University of North Carolina at Chapel Hill (UNC), and Michigan State University (MSU).Hsieh, Henry H. et al. | 2013
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DEEP LBT/LUCI SPECTROSCOPY OF AN Lyα EMITTER CANDIDATE AT z 7.7The LBT is an international collaboration among institutions in the United States, Italy, and Germany. LBT Corporation partners are: The University of Arizona on behalf of the Arizona University system; Istituto Nazionale di Astrofisica, Italy; LBT Beteiligungsgesellschaft, Germany, representing the Max-Planck Society, the Astrophysical Institute Potsdam, and Heidelberg University; The Ohio State University, and The Research Corporation, on behalf of The University of Notre Dame, University of Minnesota, and University of Virginia.Jiang, Linhua et al. | 2013
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HIGH PRECISION K-SHELL PHOTOABSORPTION CROSS SECTIONS FOR ATOMIC OXYGEN: EXPERIMENT AND THEORYMcLaughlin, B. M. et al. | 2013
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DISTRIBUTION OF PLASMOIDS IN POST-CORONAL MASS EJECTION CURRENT SHEETSGuo, L.-J. et al. | 2013
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NAVY PRECISION OPTICAL INTERFEROMETER OBSERVATIONS OF THE EXOPLANET HOST κ CORONAE BOREALIS AND THEIR IMPLICATIONS FOR THE STAR'S AND PLANET'S MASSES AND AGESBaines, Ellyn K. et al. | 2013
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SUPERNOVA EXPLOSIONS OF SUPER-ASYMPTOTIC GIANT BRANCH STARS: MULTICOLOR LIGHT CURVES OF ELECTRON-CAPTURE SUPERNOVAETominaga, Nozomu et al. | 2013
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A NOVEL APPROACH IN THE WEAKLY INTERACTING MASSIVE PARTICLE QUEST: CROSS-CORRELATION OF GAMMA-RAY ANISOTROPIES AND COSMIC SHEARCamera, Stefano et al. | 2013
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DISCOVERY OF AN EXTRA HARD SPECTRAL COMPONENT IN THE HIGH-ENERGY AFTERGLOW EMISSION OF GRB 130427ATam, Pak-Hin Thomas et al. | 2013
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SUPERNOVA EJECTA IN THE YOUNGEST GALACTIC SUPERNOVA REMNANT G1.9+0.3Borkowski, Kazimierz J. et al. | 2013
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A DYNAMICAL SIGNATURE OF MULTIPLE STELLAR POPULATIONS IN 47 TUCANAERicher, Harvey B. et al. | 2013
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VELOCITY AND MAGNETIC FIELD DISTRIBUTION IN A FORMING PENUMBRARomano, P. et al. | 2013
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IMPROVED DETERMINATION OF THE 10-00 ROTATIONAL FREQUENCY OF NH3D+ FROM THE HIGH-RESOLUTION SPECTRUM OF THE ν4 INFRARED BANDDoménech, J. L. et al. | 2013
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ERRATUM: "DYNAMICAL EVIDENCE FOR A MAGNETOCENTRIFUGAL WIND FROM A 20 MBINARY YOUNG STELLAR OBJECT" (2013, ApJL, 770, L32)Greenhill, L. J. et al. | 2013
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A COSMIC MICROWAVE BACKGROUND LENSING MASS MAP AND ITS CORRELATION WITH THE COSMIC INFRARED BACKGROUNDHolder, G. P. et al. | 2013