The evolution of massive stars: bridging the gap in the Local Group.The Effective Temperature Scale of Galactic Red Supergiants: Cool, but Not as Cool as We ThoughtThe physical properties of the red supergiant WOH G64: the largest star known?The Effective Temperatures and Physical Properties of Magellanic Cloud Red Supergiants: The Effects of MetallicityBringing VY Canis Majoris Down to Size: An Improved Determination of Its Effective TemperatureThe Red Supergiant Content of the Local GroupImpact of mass-loss on the evolution and pre-supernova properties of red supergiantsDiscovery of a Thorne-Żytkow object candidate in the Small Magellanic CloudDiscovery of a Thorne–Żytkow object candidate in the Small Magellanic CloudSpectral types of red supergiants in NGC 6822 and the Wolf-Lundmark-Melotte galaxyGrids of stellar models with rotationRed supergiants in the Andromeda galaxy (M31)Dust around red supergiants in the Magellanic CloudsThe Physical Properties of Red Supergiants: Comparing Theory and ObservationsLate‐Type Red Supergiants: Too Cool for the Magellanic Clouds?HV 11423: The Coolest Supergiant in the SMCThe Reddening of Red Supergiants: When Smoke Gets in Your EyesSN 2010ay IS A LUMINOUS AND BROAD-LINED TYPE Ic SUPERNOVA WITHIN A LOW-METALLICITY HOST GALAXYVariable Lyα sheds light on the environment surrounding GRB 090426A panchromatic view of the restless SN 2009ip reveals the explosive ejection of a massive star envelopeA spectroscopic study of type ibc supernova host galaxies from untargeted surveysSUPERNOVA 2008bk AND ITS RED SUPERGIANT PROGENITORSN 2009bb: A PECULIAR BROAD-LINED TYPE Ic SUPERNOVA,SPIRITS: Uncovering Unusual Infrared Transients with SpitzerPhysical Properties of II Zw 40's Super Star Cluster and Nebula: New Insights and Puzzles from UV SpectroscopyGRBâ 090426: the environment of a rest-frame 0.35-s gamma-ray burst at a redshift of 2.609A missing-link in the Supernova-GRB connection: the case of SN 2012apALMA observations of the host galaxy of GRB 090423 at z = 8.23: deep limits on obscured star formation 630 million years after the Big BangSN 2012au: A GOLDEN LINK BETWEEN SUPERLUMINOUS SUPERNOVAE AND THEIR LOWER-LUMINOSITY COUNTERPARTSPanchromatic observations of SN 2011dh point to a compact progenitor starSimulations of Jets in Dynamic Galaxy Cluster AtmospheresThe answer is blowing in the wind: simulating the interaction of jets with dynamic cluster atmospheresHost galaxy properties of the subluminous GRB 120422A/SN 2012bzMetallicity in the GRB 100316D/SN 2010bh host complexNew Beryllium results in halo stars from Keck/HIRES spectraBeryllium in the Oldest StarsThe high-metallicity explosion environment of the relativistic supernova 2009bbThe peculiar Balmer decrement of SN 2009ip: constraints on circumstellar geometryDetection of three gamma-ray burst host galaxies at z ~ 6GRB 070714B--Discovery of the highest spectroscopically confirmed short burst redshift
P50
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P50
description
American astrophysicist
@en
Amerikaans astrofysica
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astrofísica estadounidense
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astrophysicienne américaine
@fr
réaltfhisiceoir Meiriceánach
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name
Emily Levesque
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Emily Levesque
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Emily Levesque
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Emily Levesque
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Emily Levesque
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Emily Levesque
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Emily Levesque
@sl
אמילי לבק
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艾蜜莉·李維斯克
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type
label
Emily Levesque
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Emily Levesque
@en
Emily Levesque
@es
Emily Levesque
@fr
Emily Levesque
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Emily Levesque
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Emily Levesque
@sl
אמילי לבק
@he
艾蜜莉·李維斯克
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prefLabel
Emily Levesque
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Emily Levesque
@en
Emily Levesque
@es
Emily Levesque
@fr
Emily Levesque
@ga
Emily Levesque
@nl
Emily Levesque
@sl
אמילי לבק
@he
艾蜜莉·李維斯克
@zh
P106
P1412
P1559
Emily Levesque
@en
P19
P21
P31
P569
1950-01-01T00:00:00Z