Results 161 to 170 of about 29,281 (217)

Photon strength functions and nuclear level densities: invaluable input for nucleosynthesis. [PDF]

Philos Trans A Math Phys Eng Sci
Wiedeking M, Goriely S.
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Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Our Galaxy. [PDF]

Open Res Eur
Klaassen P, Traficante A, Beltrán M, Pattle K, Booth M, Lovell J, Marshall J, Hacar A, Gaches B, Bot C, Peretto N, Stanke T, Arzoumanian D, Duarte Cabral A, Duchêne G, Eden D, Hales A, Kauffmann J, Luppe P, Marino S, Redaelli E, Rigby A, Sánchez-Monge Á, Schisano E, Semenov D, Spezzano S, Thompson M, Wyrowski F, Cicone C, Mroczkowski T, Cordiner M, Di Mascolo L, Johnstone D, van Kampen E, Lee M, Liu D, Maccarone T, Saintonge A, Smith M, Thelen A, Wedemeyer S.   +40 more
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Genomes of Galápagos Mockingbirds Reveal the Impact of Island Size and Past Demography on Inbreeding and Genetic Load in Contemporary Populations. [PDF]

Mol Ecol
Vlček J, Espinoza-Ulloa S, Cowles SA, Ortiz-Catedral L, Coutu C, Chaves JA, Andrés J, Štefka J.   +7 more
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A high-quality genome assembly of Annona squamosa (custard apple) provides functional insights into an emerging fruit crop. [PDF]

DNA Res
Bisht MS, Mahajan S, Chakraborty A, Sharma VK.   +3 more
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Galactic supernova remnants

Space Science Reviews, 1985
A progress report is given on our current interpretation of the X-ray emission from supernova remnants. Previous results from earlier experiments, the Einstein Observatory in particular, are reviewed and supplemented by the most recent data from the Exosat mission for a selection of remnants (Puppis-A, Cas-A, SN 1006, RCW103, W49B).
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Supernovae and Supernova Remnants

1983
Supernovae are the result of explosions which terminate the life of massive stars. The amount of energy released by the supernovae in our galaxy is so large that these explosions provide the dominant energy for the heating of the hot (T ≳ 106 K) IS component and for the kinetic energy of the large scale motions of the interstellar clouds.
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Pulsar Supernova Remnant Correlation

Communications in Theoretical Physics, 1986
A formula is provided to check the correlation of pulsars and supernova remnants, using only observable pulsar parameters. The validity of this formula depends on the assumption that the value of the initial pulsar frequency is much greater than the present value. A test for this assumption is suggested.
A Qadir, M Rafique
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Barrel-like Supernova Remnants

Publications of the Astronomical Society of Australia, 1990
AbstractThe origin of cylindrically symmetric supernova remnants (SNR) is discussed. The results of numerical simulations of the two best examples of barrel-like SNRs, SN 1006 and G296.5+10.0, are presented.
G. S. Bisnovatyi-Kogan, T. A. Lozinskaya, S. A. Silich   +2 more
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Supernova remnants

Symposium - International Astronomical Union, 1967
The brightness distribution of the remnant of Tycho's Nova, which Baldwin has shown in Paper 56 (Figure 6), and the distance of 5000 pc determined by Menon and Williams (unpublished), establish beyond doubt a diameter of 10·8 pc and an average velocity of 13 300 km/sec. The initial velocity must have been higher.
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