activity
20072023
most citedCfA3: 185 Type Ia Supernova Light Curves from the CfA

524 citations · 2.9k across the 29 of their papers we have counts for

collaborators

29 papers

astro-ph.EP2023★ 21 cited

Orbital alignment of the eccentric warm Jupiter TOI-677 b

Elyar Sedaghati, Andrés Jordán, Rafael Brahm +3

Warm Jupiters lay out an excellent laboratory for testing models of planet formation and migration. Their separation from the host star makes tidal reprocessing of their orbits ine…

astro-ph.EP2023★ 24 cited

Three long period transiting giant planets from TESS

Rafael Brahm, Solène Ulmer-Moll, Melissa J. Hobson +52

We report the discovery and orbital characterization of three new transiting warm giant planets. These systems were initially identified as presenting single transit events in the…

astro-ph.HE2022★ 2 cited

Circumbinary Accretion: From Binary Stars to Massive Binary Black Holes

Dong Lai, Diego J. Muñoz

We review recent works on the dynamics of circumbinary accretion, including time variability, angular momentum transfer between the disk and the binary, and the secular evolution o…

astro-ph.HE2022

Eccentric Mergers of Intermediate-Mass Black Holes from Evection Resonances in AGN Disks

Diego J. Muñoz, Nicholas C. Stone, Cristobal Petrovich +1

We apply the theory of nonlinear resonance capture to the problem of a black hole binary (BHB) orbiting a supermassive black hole (SMBH) while embedded in the accretion disk of an…

astro-ph.HE2022★ 62 cited

Preferential Accretion and Circumbinary Disk Precession in Eccentric Binary Systems

Magdalena Siwek, Rainer Weinberger, Diego Munoz +1

We present a suite of high resolution hydrodynamic simulations of binaries immersed in circumbinary accretion disks (CBDs). For the first time, we investigate the preferential accr…

astro-ph.EP2021★ 32 cited

Outward Migration of Super-Jupiters

Adam M. Dempsey, Diego J. Muñoz, Yoram Lithwick

Recent simulations show that giant planets of about one Jupiter mass migrate inward at a rate that differs from the Type II prediction. Here we show that at higher masses, planets…