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researcher

T. Hirota

152 papers hereh-index 426.8k citations310 works total

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

author position
  • sole author1
  • first author21
  • middle author112
  • last author3

Across the 137 of 152 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA60
  • astro-ph.SR58
  • astro-ph19
  • astro-ph.HE6
  • astro-ph.IM6
  • astro-ph.EP3
same name
  • T. Hirota — 11 papers, h 3
  • T. Hirota — 1 paper, h 2
  • T. Hirota — 1 paper, h 1
  • T. Hirota — 1 paper

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
20012026
most citedTrigonometric Parallaxes of Massive Star Forming Regions: VI. Galactic Structure, Fundamental Parameters and Non-Circular Motions

1.1k citations · 6.8k across the 150 of their papers we have counts for

collaborators
Showing astro-ph.EPShow all

3 papers · 1 filter

astro-ph.EP2018★ 22 cited

Candidate Water Vapor Lines to Locate the H2​O Snowline through High-dispersion Spectroscopic Observations. III. Submillimeter H2​16O and H2​18O Lines

Shota Notsu, Hideko Nomura, Catherine Walsh +4

In this paper, we extend the results presented in our former papers (Notsu et al. 2016, 2017) on using ortho-H2​16O line profiles to constrain the location…

astro-ph.EP2017★ 45 cited

Candidate Water Vapor Lines to Locate the H2​O Snowline through High-Dispersion Spectroscopic Observations II. The Case of a Herbig Ae Star

Shota Notsu, Hideko Nomura, Daiki Ishimoto +4

Observationally measuring the location of the H2​O snowline is crucial for understanding the planetesimal and planet formation processes, and the origin of water on Earth. In d…

astro-ph.EP2016★ 43 cited

Candidate Water Vapor Lines to Locate the H2​O Snowline through High-Dispersion Spectroscopic Observations I. The Case of a T Tauri Star

Shota Notsu, Hideko Nomura, Daiki Ishimoto +4

Inside the H2​O snowline of protoplanetary disks, water evaporates from the dust-grain surface into the gas phase, whereas it is frozen out on to the dust in the cold region be…

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