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researcher

H. Yamamoto

66 papers hereh-index 283.1k citations100 works total

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

author position
  • first author4
  • middle author52
  • last author3

Across the 59 of 66 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA44
  • astro-ph.HE10
  • astro-ph5
  • astro-ph.SR4
  • astro-ph.CO2
  • astro-ph.IM1
same name
  • H. Yamamoto — 144 papers, h 82
  • H. Yamamoto — 63 papers, h 29
  • H. Yamamoto — 54 papers
  • H. Yamamoto — 51 papers
  • H. Yamamoto — 27 papers, h 25
  • H. Yamamoto — 24 papers, h 12

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
20062026
most citedObservations of the young supernova remnant RX J1713.7-3946 with the Fermi Large Area Telescope

239 citations · 2.6k across the 66 of their papers we have counts for

collaborators
Showing 2016Show all

3 papers · 1 filter

astro-ph.HE2016★ 2 cited

Interstellar Gas and X-rays toward the Young Supernova Remnant RCW 86; Pursuit of the Origin of the Thermal and Non-Thermal X-ray

H. Sano, E. M. Reynoso, I. Mitsuishi +13

We have analyzed the atomic and molecular gas using the 21 cm HI and 2.6/1.3 mm CO emissions toward the young supernova remnant (SNR) RCW 86 in order to identify the interstellar m…

astro-ph.GA2016★ 51 cited

Kinematic Structure of Molecular Gas around High-mass Star YSO, Papillon Nebula, in N159 East in the Large Magellanic Cloud

Kazuya Saigo, Toshikazu Onishi, Omnarayani Nayak +20

We present the ALMA Band 3 and Band 6 results of 12CO(2-1), 13$CO(2-1), H30alpha recombination line, free-free emission around 98 GHz, and the dust thermal emission around 230 GHz…

astro-ph.GA2016★ 16 cited

A massive molecular outflow in the dense dust core AGAL G337.916-00.477

Kazufumi Torii, Yusuke Hattori, Keisuke Hasegawa +9

Massive molecular outflows erupting from high-mass young stellar objects provide important clues to understanding the mechanism of high-mass star formation. Based on new CO J=3-2 a…

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