نتائج البحث - "W. D. Taylor"

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دورية أكاديمية

Comparative study of fungal stability between Metarhizium strains after successive subculture

المؤلفون: Rana H. M. Hussien, Said M. Ezzat, Ali A. El Sheikh, James W. D. Taylor, Tariq M. Butt

المصدر: Egyptian Journal of Biological Pest Control, Vol 31, Iss 1, Pp 1-6 (2021)

مصطلحات موضوعية: Fungal stability, Metarhizium strains, Pr1, Virulence, Agriculture

وصف الملف: electronic resource

Relation: https://doaj.org/toc/2536-9342

URL الوصول: https://doaj.org/article/dc5c53ffcab548aab911c27da92ddc84

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The B-type binaries characterization programme I

المؤلفون: S. E. de Mink, J. I. Villaseñor, O. H. Ramirez-Agudelo, Chris Evans, Norbert Langer, W. D. Taylor, Hugues Sana, Leonardo A. Almeida, Philip Dufton

المساهمون: Low Energy Astrophysics (API, FNWI)

المصدر: Villaseñor, J I, Taylor, W D, Evans, C J, Ramírez-Agudelo, O H, Sana, H, Almeida, L A, de Mink, S E, Dufton, P L & Langer, N 2021, ' The B-type binaries characterization programme I. Orbital solutions for the 30 Doradus population ', Monthly Notices of the Royal Astronomical Society, vol. 507, no. 4, pp. 5348-5375 . https://doi.org/10.1093/mnras/stab2197
Monthly Notices of the Royal Astronomical Society, 507(4), 5348-5375. Oxford University Press

مصطلحات موضوعية: ULTRAVIOLET, Population, ECLIPSING BINARY, FOS: Physical sciences, Binary number, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astronomy & Astrophysics, spectroscopic [binaries], early-type [stars], massive [stars], individual: 30 Doradus [open clusters and associations], Magellanic Clouds, Astrophysics::Solar and Stellar Astrophysics, education, Large Magellanic Cloud, Solar and Stellar Astrophysics (astro-ph.SR), Astrophysics::Galaxy Astrophysics, Physics, education.field_of_study, Science & Technology, FLAMES TARANTULA SURVEY, MULTIPLICITY, OBSERVATIONAL CAMPAIGN, Astronomy and Astrophysics, PULSAR, stars: early-type, ROTATIONAL VELOCITIES, galaxies: Magellanic Clouds, Galaxy, stars: massive, Black hole, VARIABILITY, Stars, Supernova, open clusters and associations: individual: 30 Doradus, Astrophysics - Solar and Stellar Astrophysics, Space and Planetary Science, Physical Sciences, BLACK-HOLE, Probability distribution, binaries: spectroscopic, MASSIVE STARS

وصف الملف: application/pdf

URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f622b586b26c4a46fb0dc3a3d860693f
https://doi.org/10.1093/mnras/stab2197

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Properties of the Be-type stars in 30 Doradus

المؤلفون: P L Dufton, D J Lennon, J I Villaseñor, I D Howarth, C J Evans, S E de Mink, H Sana, W D Taylor

المصدر: Dufton, P L, Lennon, D J, Villaseñor, J I, Howarth, I D, Evans, C J, de Mink, S E, Sana, H & Taylor, W D 2022, ' Properties of the Be-type stars in 30 Doradus ', Monthly Notices of the Royal Astronomical Society, vol. 512, no. 3, pp. 3331-3344 . https://doi.org/10.1093/mnras/stac630

مصطلحات موضوعية: SAMPLE, star clusters: individual: Tarantula Nebula [galaxies], FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astronomy & Astrophysics, PARAMETERS, TESS OBSERVATIONS, Magellanic Clouds, Astrophysics::Solar and Stellar Astrophysics, SMALL-MAGELLANIC-CLOUD, FIELD, SUPERGIANTS, POPULATION, Astrophysics::Galaxy Astrophysics, Solar and Stellar Astrophysics (astro-ph.SR), Science & Technology, Astronomy and Astrophysics, ROTATIONAL VELOCITIES, Astrophysics - Astrophysics of Galaxies, STELLAR, Astrophysics - Solar and Stellar Astrophysics, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Physical Sciences, rotation [stars], emission-line, Be [stars], Astrophysics::Earth and Planetary Astrophysics, MASSIVE STARS