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researcher

M. Otsuka

44 papers hereh-index 201.3k citations93 works total

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

author position
  • sole author1
  • first author13
  • middle author17
  • last author9

Across the 40 of 44 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR22
  • astro-ph.GA12
  • astro-ph3
  • astro-ph.CO3
  • astro-ph.HE3
  • astro-ph.IM1
same name
  • M. Otsuka — 5 papers
  • M. Otsuka — 4 papers, h 4
  • M. Otsuka — 3 papers, h 4
  • M. Otsuka — 1 paper, h 1
  • M. Otsuka — 1 paper, h 1
  • M. Otsuka — 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
20062023
most citedHerschel Detects a Massive Dust Reservoir in Supernova 1987A

368 citations · 1.3k across the 44 of their papers we have counts for

collaborators
Showing 2023Show all

3 papers · 1 filter

astro-ph.GA2023

Seimei KOOLS-IFU mapping of the gas and dust distributions in Galactic PNe: Unveiling the origin and evolution of Galactic halo PN H4-1

Masaaki Otsuka, Toshiya Ueta, Akito Tajitsu

H4-1 is a planetary nebula (PN) located in the Galactic halo, and is notably carbon-rich and one of the most metal-deficient PNe in the Milky Way. To unveil its progenitor evolutio…

astro-ph.GA2023

Probing the origin of the two-component structure of broad line region by reverberation mapping of an extremely variable quasar

Shumpei Nagoshi, Fumihide Iwamuro, Satoshi Yamada +5

The physical origins of quasar components, such as the broad line region (BLR) and dust torus, remain under debate. To gain insights into them, we focused on Changing-State Quasars…

astro-ph.SR2023

The messy death of a multiple star system and the resulting planetary nebula as observed by JWST

Orsola De Marco, Muhammad Akashi, Stavros Akras +66

Planetary nebulae (PNe), the ejected envelopes of red giant stars, provide us with a history of the last, mass-losing phases of 90 percent of stars initially more massive than the…

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