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N. Hirano

107 papers hereh-index 384.2k citations186 works total

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

author position
  • first author7
  • middle author81
  • last author8

Across the 96 of 107 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA56
  • astro-ph.SR29
  • astro-ph20
  • astro-ph.EP2
same name
  • N. Hirano — 14 papers, h 5
  • N. Hirano — 2 papers, h 18

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
19992024
most citedImaging the Disk around TW Hya with the Submillimeter Array

204 citations · 3.6k across the 107 of their papers we have counts for

collaborators
Showing 2010Show all

4 papers · 1 filter

astro-ph.GA2010★ 14 cited

Chemical Variation in Molecular Cloud Cores in the Orion A Cloud

Ken'ichi Tatematsu, Tomoya Hirota, Ryo Kandori +1

We have observed molecular cloud cores in the Orion A giant molecular cloud (GMC) in CCS, HC3N, DNC, and HN13C to study their chemical characteristics. We have detected CCS in the…

astro-ph.SR2010★ 115 cited

Extreme Active Molecular Jets in L1448C

Naomi Hirano, Paul P. T. Ho, Sheng-Yuan Liu +3

The protostellar jet driven by L1448C was observed in the SiO J=8-7 and CO J=3-2 lines and 350 GHz dust continuum at ~1" resolution with the Submillimeter Array (SMA). A narrow jet…

astro-ph.GA2010★ 69 cited

The reflection-symmetric wiggle of the young protostellar jet HH 211

Chin-Fei Lee, Tatsuhiko I. Hasegawa, Naomi Hirano +4

HH 211 is a highly collimated jet originating from a nearby young Class 0 protostar. Here is a follow-up study of the jet with our previous observations at unprecedented resolution…

astro-ph.GA2010★ 15 cited

Outflow - Core Interaction in Barnard 1

Masaaki Hiramatsu, Naomi Hirano, Shigehisa Takakuwa

In order to study how outflows from protostars influence the physical and chemical conditions of the parent molecular cloud, we have observed Barnard 1 (B1) main core, which harbor…

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