1 citations · 1 across the 4 of their papers we have counts for
5 papers
Towards A Universal Analytical Model of Population III Star Formation: A Bridge Between Cosmological Scales and Protostars
James Gurian, Boyuan Liu, Donghui Jeong +4
We construct an analytical model of Population III star formation that connects the cosmological radiation background to sub-AU protostellar disk fragmentation, a dynamic range ina…
Simulations of multiple dust ring formation in a subsolar-metallicity protoplanetary disk
Ryoki Matsukoba, Eduard I. Vorobyov, Takashi Hosokawa
Super-Earths exist around subsolar-metallicity host stars with a frequency comparable to that around solar-metallicity stars, suggesting efficient assembly of dust grains even in m…
Planet Formation at Cosmic Dawn: Planetesimals in HO-Rich Disks Around Low-Mass Stars
Eduard I. Vorobyov, Daniel J. Whalen, Muhammad A. Latif +5
Primordial, or Pop III, supernovae (SNe) were the first, great nucleosynthetic engines in the Universe, forging the heavy elements required for the later formation of planets, and…
Secret of Longevity: Protoplanetary Disks as a Source of Gas in Debris Disks
Wataru Ooyama, Riouhei Nakatani, Takashi Hosokawa +2
While protoplanetary disks (PPDs) are generally thought to disperse within several million years, recent observations have revealed gas in their older counterparts, debris disks. T…
Metallicity dependence of dust growth in a protoplanetary disk
Ryoki Matsukoba, Eduard I. Vorobyov, Takashi Hosokawa
In the context of planet formation, growth from micron-sized grains to kilometer-sized planetesimals is a crucial question. Since the dust growth rate depends on the amount of dust…