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researcher

S. Takahashi

29 papers hereh-index 17952 citations36 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author9
  • middle author17
  • last author3

Across the 29 of 29 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP13
  • astro-ph.SR11
  • astro-ph.GA4
  • astro-ph.HE1
same name
  • S. Takahashi — 36 papers, h 44
  • S. Takahashi — 29 papers, h 20
  • S. Takahashi — 25 papers, h 36
  • S. Takahashi — 9 papers, h 18
  • S. Takahashi — 7 papers, h 11
  • S. Takahashi — 7 papers, h 7

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20132026
most citedFormation of a Keplerian disk in the infalling envelope around L1527 IRS: transformation from infalling motions to Kepler motions

194 citations · 1.3k across the 29 of their papers we have counts for

collaborators
Showing 2013Show all

3 papers · 1 filter

astro-ph.EP2013★ 182 cited

Two-Component Secular Gravitational Instability in a Protoplanetary Disk: A Possible Mechanism for Creating Ring-Like Structures

Sanemichi Z. Takahashi, Shu-ichiro Inutsuka

The instability in protoplanetary disks due to gas-dust friction and self-gravity of gas and dust is investigated by linear analysis. In the case where the dust to gas ratio is enh…

astro-ph.SR2013★ 154 cited

Local Enhancement of Surface Density in the Protoplanetary Ring Surrounding HD 142527

Misato Fukagawa, Takashi Tsukagoshi, Munetake Momose +15

We report ALMA observations of dust continuum, 13CO J=3--2, and C18O J=3--2 line emission toward a gapped protoplanetary disk around HD 142527. The outer horseshoe-shaped disk show…

astro-ph.SR2013★ 49 cited

A Semi-Analytical Description for the Formation and Gravitational Evolution of Protoplanetary Disks

Sanemichi Z. Takahashi, Shu-ichiro Inutsuka, Masahiro N. Machida

We investigate the formation process of self-gravitating protoplanetary disks in unmagnetized molecular clouds. The angular momentum is redistributed by the action of gravitational…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.