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20022026
most citedSuper-critical Accretion Flows around Black Holes: Two-dimensional, Radiation-pressure-dominated Disks with Photon-trapping

443 citations · 1.4k across the 26 of their papers we have counts for

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6 papers · 1 filter

astro-ph2008★ 33 cited

Observational Possibility of the "Snow Line" on the Surface of Circumstellar Disks with the Scattered Light

Akio K. Inoue, Mitsuhiko Honda, Taishi Nakamoto +1

We discuss how we obtain the spatial distribution of ice on the surface of the circumstellar disk around young stars. Ice in the disks plays a very important role in various issues…

astro-ph2006★ 23 cited

Shock-Wave Heating Model for Chondrule Formation: Prevention of Isotopic Fractionation

Hitoshi Miura, Taishi Nakamoto

Chondrules are considered to have much information on dust particles and processes in the solar nebula. It is naturally expected that protoplanetary disks observed in present star…

astro-ph2006★ 222 cited

Cosmological Radiative Transfer Codes Comparison Project I: The Static Density Field Tests

Ilian T. Iliev, Benedetta Ciardi, Marcelo A. Alvarez +13

Radiative transfer simulations are now at the forefront of numerical astrophysics. They are becoming crucial for an increasing number of astrophysical and cosmological problems; at…

astro-ph2005★ 443 cited

Super-critical Accretion Flows around Black Holes: Two-dimensional, Radiation-pressure-dominated Disks with Photon-trapping

K. Ohsuga, M. Mori, T. Nakamoto +1

The quasi-steady structure of super-critical accretion flows around a black hole is studied based on the two-dimensional radiation-hydrodynamical (2D-RHD) simulations. The super-cr…

astro-ph2002★ 9 cited

A Spectrophotometric Method to Determine the Inclination of Class I Objects

T. Nakazato, T. Nakamoto, M. Umemura

A new method which enables us to estimate the inclination of Class I young stellar objects is proposed. Since Class I objects are not spherically symmetric, it is likely that the o…

astro-ph2002★ 12 cited

Disk-Halo Model for Flat-Spectrum T Tauri Stars

N. Kikuchi, T. Nakamoto, K. Ogochi

We explore the origin of the flat spectrum seen in some T Tauri stars by considering a three-component structure: a central star, a circumstellar disk, and a dusty halo. The radiat…