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researcher

M. Sato

3 papers hereh-index 447 citations10 works total

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

author position
  • middle author2
  • last author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
same name
  • M. Sato — 100 papers, h 57
  • M. Sato — 17 papers, h 14
  • M. Sato — 14 papers, h 15
  • M. Sato — 7 papers, h 16
  • M. Sato — 7 papers, h 20
  • M. Sato — 6 papers, h 15

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

most citedThe Opaque Heart of the Galaxy IC 860: Analogous Protostellar, Kinematics, Morphology, and Chemistry

12 citations · 17 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2024★ 5 cited

A spectacular galactic scale magnetohydrodynamic powered wind in ESO 320-G030

M. D. Gorski, S. Aalto, S. König +23

How galaxies regulate nuclear growth through gas accretion by supermassive black holes (SMBHs) is one of the most fundamental questions in galaxy evolution. One potential way to re…

astro-ph.GA2024

Double, double, toil, and trouble: The tails, bubbles, and knots of the local compact obscured nucleus galaxy NGC4418

C. F. Wethers, S. Aalto, G. C. Privon +20

Compact obscured nuclei (CONs) are an extremely obscured (NH2​ >1025 cm−2) class of galaxy nuclei thought to exist in 20-40 per cent of nearby (ultra-)luminous infrar…

astro-ph.GA2022★ 12 cited

The Opaque Heart of the Galaxy IC 860: Analogous Protostellar, Kinematics, Morphology, and Chemistry

M. D. Gorski, S. Aalto, S. König +7

Compact Obscured Nuclei (CONs) account for a significant fraction of the population of luminous and ultraluminous infrared galaxies (LIRGs and ULIRGs). These galaxy nuclei are comp…

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