activity
20172022
most citedAn Ultra-Hot Neptune in the Neptune desert

85 citations · 147 across the 6 of their papers we have counts for

collaborators

17 papers

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.EP202211 cited

Mutual Inclination of Ultra-Short-Period Planets with Time Varying Stellar J2-moment

Chen Chen, Gongjie Li, Cristobal Petrovich

Systems with ultra-short-period planets (USPs) tend to possess larger mutual inclinations compared to those with planets located farther from their host stars. This could be explai…

astro-ph.GA20213 cited

Formation of counter-rotating and highly eccentric massive black hole binaries in galaxy mergers

Imran Nasim, Cristobal Petrovich, Adam Nasim +2

Supermassive black hole (SMBH) binaries represent the main target for missions such as the Laser Interferometer Space Antenna and Pulsar Timing Arrays. The understanding of their d…

astro-ph.EP202112 cited

Observable Predictions from Perturber-coupled High-eccentricity Tidal Migration of Warm Jupiters

Jonathan M. Jackson, Rebekah I. Dawson, Andrew Shannon +1

The origin of warm Jupiters (gas giant planets with periods between 10 and 200 days) is an open question in exoplanet formation and evolution. We investigate a particular migration…

astro-ph.EP2020

Kozai Migration Naturally Explains the White Dwarf Planet WD1856b

Diego J. Muñoz, Cristobal Petrovich

The Jovian-sized object WD~1856~b transits a white dwarf (WD) in a compact -day orbit. Unlikely to have endured stellar evolution in its current orbit, WD~1856~b is thought to…

astro-ph.EP202085 cited

An Ultra-Hot Neptune in the Neptune desert

James S. Jenkins, Matías R. Díaz, Nicolás T. Kurtovic +81

About one out of 200 Sun-like stars has a planet with an orbital period shorter than one day: an ultra-short-period planet (Sanchis-ojeda et al. 2014; Winn et al. 2018). All of the…