activity
20092016
most citedOn the Minimum Core Mass for Giant Planet Formation at Wide Separations

214 citations · 522 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.EP2016★ 69 cited

The Role of Ice Compositions for Snowlines and the C/N/O Ratios in Active Disks

Ana-Maria A. Piso, Jamila Pegues, Karin I. Oberg

The elemental compositions of planets define their chemistry, and could potentially be used as beacons for their formation location if the elemental gas and grain ratios of planet…

astro-ph.EP2015★ 120 cited

C/O and Snowline Locations in Protoplanetary Disks: The Effect of Radial Drift and Viscous Gas Accretion

Ana-Maria A. Piso, Karin I. Oberg, Tilman Birnstiel +1

The C/O ratio is a defining feature of both gas giant atmospheric and protoplanetary disk chemistry. In disks, the C/O ratio is regulated by the presence of snowlines of major vola…

astro-ph.EP2014★ 112 cited

Minimum Core Masses for Giant Planet Formation With Realistic Equations of State and Opacities

Ana-Maria A. Piso, Andrew N. Youdin, Ruth A. Murray-Clay

Giant planet formation by core accretion requires a core that is sufficiently massive to trigger runaway gas accretion in less that the typical lifetime of protoplanetary disks. We…

astro-ph.EP2013★ 214 cited

On the Minimum Core Mass for Giant Planet Formation at Wide Separations

Ana-Maria A. Piso, Andrew N. Youdin

In the core accretion hypothesis, giant planets form by gas accretion onto solid protoplanetary cores. The minimum (or critical) core mass to form a gas giant is typically quoted a…

astro-ph.SR2009★ 7 cited

Exact relativistic viscous fluid solutions in near horizon extremal Kerr background

Daniel Grumiller, Ana-Maria Piso

Realistic accretion disk models require a number of ingredients, including viscous fluids, electromagnetic fields and general relativistic corrections. Close to the innermost stabl…