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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 2013Show all

3 papers · 1 filter

astro-ph.SR2013★ 44 cited

Observations of 6.7 GHz Methanol Masers with EAVN I: VLBI Images of the first Epoch of Observations

Kenta Fujisawa, Koichiro Sugiyama, Kazuhito Motogi +26

Very long baseline interferometry (VLBI) monitoring of the 6.7 GHz methanol maser allows us to measure the internal proper motions of the maser spots and therefore study the gas mo…

astro-ph.GA2013★ 18 cited

Chemical Variation in Molecular Cloud Cores in the Orion A Cloud. II

Ken'ichi Tatematsu, Satoshi Ohashi, Tomofumi Umemoto +6

We have mapped six molecular cloud cores in the Orion A giant molecular cloud (GMC), whose kinetic temperatures range from 10 to 30 K, in CCS and N2H+ with Nobeyama 45 m radio tele…

astro-ph.SR2013★ 38 cited

ALMA Observations of the IRDC Clump G34.43+00.24 MM3: Hot Core and Molecular Outflows

Takeshi Sakai, Nami Sakai, Jonathan B. Foster +7

We have observed a cluster forming clump (MM3) associated with the infrared dark cloud G34.43+00.24 in the 1.3 mm continuum and the CH3OH, CS, 13CS, SiO, CH3CH2CN, and HCOOCH3 line…

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