activity
19992025
most citedAn Extended Grid of Nova Models: II. The Parameter Space of Nova Outbursts

530 citations · 1.2k across the 32 of their papers we have counts for

collaborators
Showing astro-ph.EPShow all

14 papers · 1 filter

astro-ph.EP2025

Combined Orbital and Thermal Evolution of Oort Cloud Comets

Adam Parhi, Dina Prialnik

We present a fully integrated model of comet evolution that couples thermal and compositional processes with dynamical processes continuously, from formation to present-day activit…

astro-ph.EP2023★ 20 cited

Sublimation of ices during the early evolution of Kuiper belt objects

Adam Parhi, Dina Prialnik

Kuiper belt objects, such as Arrokoth, the probable progenitors of short-period comets, formed and evolved at large heliocentric distances, where the ambient temperatures appear to…

astro-ph.EP2023★ 3 cited

About the loss of a primordial atmosphere of super-Earths by planetesimal impacts

Michael Lozovsky, Dina Prialnik, Morris Podolak

We consider planets composed of water ice and rock, located far from a central star. In an earlier study, computing the growth of planets by continuous accretion, we found that a l…

astro-ph.EP2022

29P/Schwassmann-Wachmann: A Rosetta Stone for Amorphous Water Ice and CO <-> CO2 Conversion in Centaurs and Comets?

C. M. Lisse, J. K. Steckloff, D. Prialnik +12

Centaur 29P/Schwassmann-Wachmann 1 (SW1) is a highly active object orbiting in the transitional Gateway region (Sarid et al. 2019) between the Centaur and Jupiter Family Comet regi…

astro-ph.EP2022★ 9 cited

Amorphous ice in comets: evidence and consequences

Dina Prialnik, David Jewitt

Ice naturally forms in the disordered or ``amorphous'' state when accreted from vapor at temperatures and pressures found in the interstellar medium and in the frigid, low density…

astro-ph.EP2022★ 2 cited

The Effect of Accretion Rate and Composition on the Structure of Ice-rich Super-Earths

Michael Lozovsky, Dina Prialnik, Morris Podolak

It is reasonable to assume that the structure of a planet and the interior distribution of its components are determined by its formation history. We thus follow the growth of a pl…