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researcher

S. Mori

20 papers hereh-index 10298 citations21 works total

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

author position
  • first author4
  • middle author11
  • last author3

Across the 18 of 20 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP12
  • astro-ph.SR5
  • astro-ph.GA3
same name
  • S. Mori — 38 papers, h 11
  • S. Mori — 16 papers, h 34
  • S. Mori — 12 papers, h 31
  • S. Mori — 11 papers, h 24
  • S. Mori — 8 papers, h 13
  • S. Mori — 6 papers, h 9

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
20202026
most citedEarly Planet Formation in Embedded Disks (eDisk). I. Overview of the Program and First Results

159 citations · 493 across the 19 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2023★ 17 cited

Insights on the Sun birth environment in the context of star-cluster formation in hub-filament systems

Doris Arzoumanian, Sota Arakawa, Masato I. N. Kobayashi +7

Cylindrical molecular filaments are observed to be the main sites of Sun-like star formation, while massive stars form in dense hubs, at the junction of multiple filaments. The rol…

astro-ph.GA2022★ 22 cited

Hot methanol in the [BHB2007] 11 protobinary system: hot corino versus shock origin? : FAUST V

C. Vastel, F. Alves, C. Ceccarelli +63

Methanol is a ubiquitous species commonly found in the molecular interstellar medium. It is also a crucial seed species for the building-up of the chemical complexity in star formi…

astro-ph.GA2022★ 32 cited

FAUST III. Misaligned rotations of the envelope, outflow, and disks in the multiple protostellar system of VLA 1623−2417

Satoshi Ohashi, Claudio Codella, Nami Sakai +69

We report a study of the low-mass Class-0 multiple system VLA 1623AB in the Ophiuchus star-forming region, using H13CO+ (J=3−2), CS (J=5−4), and CCH (N=3−2) lines as…

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