activity
20132023
most citedOutflow-Confined H II Regions. I. First Signposts of Massive Star Formation

81 citations · 954 across the 39 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

12 papers · 1 filter

astro-ph.SR2023

Chemical evolution of some selected complex organic molecules in low-mass star-forming regions

Bratati Bhat, Rumela Kar, Suman Kumar Mondal +6

The destiny of complex organic molecules (COMs) in star-forming regions is interlinked with various evolutionary phases. Therefore, identifying these species in diversified environ…

astro-ph.SR2020★ 1 cited

Protostellar collapse: regulation of the angular momentum and onset of an ionic precursor

Pierre Marchand, Kengo Tomida, Kei Tanaka +2

Through the magnetic braking and the launching of protostellar outflows, magnetic fields play a major role in the regulation of angular momentum in star formation, which directly i…

astro-ph.SR2020★ 39 cited

Salt, Hot Water, and Silicon Compounds Tracing Massive Twin Disks

Kei E. I. Tanaka, Yichen Zhang, Tomoya Hirota +9

We report results of 0.05"-resolution observations toward the O-type proto-binary system IRAS 16547-4247 with the Atacama Large Millimeter/submillimeter Array (ALMA). We present dy…

astro-ph.SR2019★ 20 cited

Discovery of a Photoionized Bipolar Outflow towards the Massive Protostar G45.47+0.05

Yichen Zhang, Kei E. I. Tanaka, Viviana Rosero +6

Massive protostars generate strong radiation feedback, which may help set the mass they achieve by the end of the accretion process. Studying such feedback is therefore crucial for…

astro-ph.SR2019★ 32 cited

Dynamics of a Massive Binary at Birth

Yichen Zhang, Jonathan C. Tan, Kei E. I. Tanaka +6

Almost all massive stars have bound stellar companions, existing in binaries or higher-order multiples. While binarity is theorized to be an essential feature of how massive stars…

astro-ph.SR2018★ 16 cited

Disk wind feedback from high-mass protostars

Jan E. Staff, Kei E. I. Tanaka, Jonathan C. Tan

We perform a sequence of 3D magnetohydrodynamic (MHD) simulations of the outflow-core interaction for a massive protostar forming via collapse of an initial cloud core of $60~{M_\o…

astro-ph.SR2018★ 29 cited

The Impact of Feedback in Massive Star Formation. II. Lower Star Formation Efficiency at Lower Metallicity

Kei E. I. Tanaka, Jonathan C. Tan, Yichen Zhang +1

We conduct a theoretical study of the formation of massive stars over a wide range of metallicities from 1e-5 to 1Zsun and evaluate the star formation efficiencies (SFEs) from pres…

astro-ph.SR2017★ 11 cited

Outflow-Confined HII regions. II. The Early Break-Out Phase

Kei E. I. Tanaka, Jonathan C. Tan, Jan E. Staff +1

In this series of papers, we model the formation and evolution of the photoionized region and its observational signatures during massive star formation. Here we focus on the early…

astro-ph.SR2016★ 74 cited

The Impact of Feedback During Massive Star Formation by Core Accretion

Kei E. I. Tanaka, Jonathan C. Tan, Yichen Zhang

We study feedback during massive star formation using semi-analytic methods, considering the effects of disk winds, radiation pressure, photoevaporation and stellar winds, while fo…

astro-ph.SR2015★ 81 cited

Outflow-Confined H II Regions. I. First Signposts of Massive Star Formation

Kei E. I. Tanaka, Jonathan C. Tan, Yichen Zhang

We present an evolutionary sequence of models of the photoionized disk-wind outflow around forming massive stars based on the Core Accretion model. The outflow is expected to be th…

astro-ph.SR2013★ 45 cited

Photoevaporation of Circumstellar Disks Revisited: The Dust-Free Case

Kei E. I. Tanaka, Taishi Nakamoto, Kazuyuki Omukai

Photoevaporation by stellar ionizing radiation is believed to play an important role in the dispersal of disks around young stars. The mass loss model for dust-free disks developed…

astro-ph.SR2013★ 66 cited

Direct diagnostics of forming massive stars: stellar pulsation and periodic variability of maser sources

Kohei Inayoshi, Koichiro Sugiyama, Takashi Hosokawa +2

The 6.7 GHz methanol maser emission, a tracer of forming massive stars, sometimes shows enigmatic periodic flux variations over several 10-100 days. In this Letter, we propose that…