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S. E. Ragan

Identifiers

  • name variant S. E. Ragan 0.60 · backfill

Papers (26)

  1. NEATH III: a molecular line survey of a simulated star-forming cloud astro-ph.GA · 2024 · author #4
  2. N$_2$H$^+$(1-0) as a tracer of dense gas in and between spiral arms astro-ph.GA · 2024 · author #2
  3. NEATH II: N$_2$H$^+$ as a tracer of imminent star formation in quiescent high-density gas astro-ph.GA · 2023 · author #4
  4. Non-Equilibrium Abundances Treated Holistically (NEATH): the molecular composition of star-forming clouds astro-ph.GA · 2023 · author #4
  5. Kinematics and stability of high-mass protostellar disk candidates at sub-arcsecond resolution -- Insights from the IRAM NOEMA large program CORE astro-ph.GA · 2023 · author #28
  6. ATLASGAL -- Star forming efficiencies and the Galactic star formation rate astro-ph.GA · 2022 · author #5
  7. The SEDIGISM survey: Molecular cloud morphology. II. Integrated source properties astro-ph.GA · 2022 · author #22
  8. The SEDIGISM survey: Molecular cloud morphology. I. Classification and star formation astro-ph.GA · 2022 · author #23
  9. The SEDIGISM survey: The influence of spiral arms on the molecular gas distribution of the inner Milky Way astro-ph.GA · 2021 · author #21
  10. Disk fragmentation in high-mass star formation. High-resolution observations towards AFGL 2591-VLA 3 astro-ph.GA · 2021 · author #27
  11. The Hi-GAL compact source catalogue -- II. The 360{\deg} catalogue of clump physical properties astro-ph.GA · 2021 · author #12
  12. The SEDIGISM survey: Molecular clouds in the inner Galaxy astro-ph.GA · 2020 · author #49
  13. SEDIGISM-ATLASGAL: Dense Gas Fraction and Star Formation Efficiency Across the Galactic Disk astro-ph.GA · 2020 · author #7
  14. Ubiquitous velocity fluctuations throughout the molecular interstellar medium astro-ph.GA · 2020 · author #25
  15. CHIMPS: Physical properties of molecular clumps across the inner Galaxy astro-ph.GA · 2019 · author #5
  16. Feedback in W49A diagnosed with radio recombination lines and models astro-ph.GA · 2018 · author #19
  17. Core fragmentation and Toomre stability analysis of W3(H2O): A case study of the IRAM NOEMA large program CORE astro-ph.GA · 2018 · author #29
  18. The role of spiral arms in Milky Way star formation astro-ph.GA · 2018 · author #1
  19. OH absorption in the first quadrant of the Milky Way as seen by THOR astro-ph.GA · 2018 · author #13
  20. Multi-temperature mapping of dust structures throughout the Galactic Plane using the PPMAP tool with Herschel Hi-GAL data astro-ph.GA · 2017 · author #4
  21. Properties of Hi-GAL clumps in the inner Galaxy]{The Hi-GAL compact source catalogue. I. The physical properties of the clumps in the inner Galaxy ($-71.0^{\circ}< \ell < 67.0^{\circ}$) astro-ph.GA · 2017 · author #21
  22. The prevalence of star formation as a function of Galactocentric radius astro-ph.GA · 2016 · author #1
  23. Earliest phases of star formation (EPoS): Dust temperature distributions in isolated starless cores astro-ph.GA · 2016 · author #9
  24. Kinematic and Thermal Structure at the onset of high-mass star formation astro-ph.SR · 2015 · author #4
  25. The dynamics and star-forming potential of the massive Galactic centre cloud G0.253+0.016 astro-ph.GA · 2014 · author #5
  26. Kinematic structure of massive star-forming regions - I. Accretion along filaments astro-ph.GA · 2014 · author #6

Mentions

  • 2406.06702 #4 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 2403.19269 #2 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 2310.06037 #4 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 2305.00020 #28 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 2307.13072 #4 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 2208.11121 #5 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 2205.02253 #22 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 2203.02504 #23 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 2110.06071 #21 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 2109.04751 #27 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 2104.04807 #12 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 1812.00758 #19 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 2012.01502 #49 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 2012.01464 #7 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 2007.01877 #25 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 1909.04714 #5 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 1803.04794 #13 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 1808.00472 #29 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 1806.08276 #1 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 1707.03808 #4 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 1706.01046 #21 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 1607.07626 #1 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 1606.04318 #9 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 1504.00262 #4 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 1404.1372 #5 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 1402.0021 #6 · arxiv_oai · confidence 0.70 S. E. Ragan
  • 1504.00262 #4 · backfill · confidence 0.70 S. E. Ragan
  • 1404.1372 #5 · backfill · confidence 0.70 S. E. Ragan
  • 1402.0021 #6 · backfill · confidence 0.70 S. E. Ragan

Frequent Coauthors