◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

S. Stuber

3 papers hereh-index 13636 citations50 works total

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

author position
  • first author1
  • middle author1
  • last author1

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

fields
  • astro-ph.GA3

identity via Semantic Scholar / OpenAlex

most citedNew Constraints on the 12CO(2-1)/(1-0) Line Ratio Across Nearby Disc Galaxies

130 citations · 194 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2022★ 26 cited

The Kiloparsec-scale Neutral Atomic Carbon Outflow in the Nearby Type-2 Seyfert Galaxy NGC 1068: Evidence for Negative AGN Feedback

Toshiki Saito, Shuro Takano, Nanase Harada +13

Active galactic nucleus (AGN) feedback is postulated as a key mechanism for regulating star formation within galaxies. Studying the physical properties of the outflowing gas from A…

astro-ph.GA2021★ 38 cited

Frequency and nature of central molecular outflows in nearby star-forming disk galaxies

Sophia K. Stuber, Toshiki Saito, Eva Schinnerer +17

Central molecular outflows in spiral galaxies are assumed to modulate their host galaxy's star formation rate by removing gas from the inner region of the galaxy. Outflows consisti…

astro-ph.GA2021★ 130 cited

New Constraints on the 12CO(2-1)/(1-0) Line Ratio Across Nearby Disc Galaxies

J. S. den Brok, D. Chatzigiannakis, F. Bigiel +18

Both the CO(2-1) and CO(1-0) lines are used to trace the mass of molecular gas in galaxies. Translating the molecular gas mass estimates between studies using different lines requi…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.