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20052026
most citedThe Effective Temperature Scale of Galactic Red Supergiants: Cool, But Not As Cool As We Thought

495 citations · 6.4k across the 97 of their papers we have counts for

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Showing 2009Show all

10 papers · 1 filter

astro-ph.GA2009

Modeling the host galaxies of long-duration gamma-ray bursts

Emily M. Levesque

We present the first results of our investigation into the ISM environments of long-duration GRB (LGRB) host galaxies. We apply a new suite of stellar population synthesis and phot…

astro-ph.SR2009★ 3 cited

The Physical Properties of Red Supergiants

Emily M. Levesque

Red supergiants (RSGs) are an evolved He-burning phase in the lifetimes of moderately high mass (10 - 25 solar mass) stars. The physical properties of these stars mark them as an i…

astro-ph.HE2009★ 37 cited

The High-Metallicity Explosion Environment of the Relativistic Supernova 2009bb

E. M. Levesque, A. M. Soderberg, R. J. Foley +23

We investigate the environment of the nearby (d ~ 40Mpc) broad-lined Type Ic supernova SN 2009bb. This event was observed to produce a relativistic outflow likely powered by a cent…

astro-ph.HE2009★ 323 cited

A Relativistic Type Ibc Supernova Without a Detected Gamma-ray Burst

A. M. Soderberg, S. Chakraborti, G. Pignata +21

Long duration gamma-ray bursts (GRBs) mark the explosive death of some massive stars and are a rare sub-class of Type Ibc supernovae (SNe Ibc). They are distinguished by the produc…

astro-ph.GA2009★ 168 cited

Theoretical Modeling of Star-Forming Galaxies I. Emission Line Diagnostic Grids for Local and Low-Metallicity Galaxies

Emily M. Levesque, Lisa J. Kewley, Kirsten L. Larson

We use the newest generation of the Starburst99/Mappings code to generate an extensive suite of models to facilitate detailed studies of star-forming galaxies and their ISM propert…

astro-ph.GA2009★ 94 cited

Red Supergiants in the Andromeda Galaxy (M31)

Philip Massey, David R. Silva, Emily M. Levesque +5

Red supergiants are a short-lived stage in the evolution of moderately massive stars (10-25Mo), and as such their location in the H-R diagram provides an exacting test of stellar e…