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researcher

T. Moller

20 papers hereh-index 9342 citations35 works total

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

author position
  • first author2
  • middle author14
  • last author1

Across the 17 of 20 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA19
  • astro-ph.SR1
same name
  • T. Moller — 4 papers, h 10
  • T. Moller — 2 papers, h 2
  • T. Moller — 1 paper, h 2
  • T. Moller — 1 paper, h 2
  • T. Moller — 1 paper, h 1

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
20152026
most citedThe physical and chemical structure of Sagittarius B2, I. Three-dimensional thermal dust and free-free continuum modeling on 100 au to 45 pc scales

154 citations · 332 across the 18 of their papers we have counts for

collaborators
Showing 2021Show all

3 papers · 1 filter

astro-ph.GA2021★ 17 cited

Disk fragmentation in high-mass star formation. High-resolution observations towards AFGL 2591-VLA 3

S. Suri, H. Beuther, C. Gieser +29

Increasing evidence suggests that, similar to their low-mass counterparts, high-mass stars form through a disk-mediated accretion process. At the same time, formation of high-mass…

astro-ph.GA2021★ 17 cited

Herschel observations of extraordinary sources: Full Herschel/HIFI molecular line survey of Sagittarius B2(M)

T. Möller, P. Schilke, A. Schmiedeke +5

We present a full analysis of a broadband spectral line survey of Sagittarius B2 (Main), one of the most chemically rich regions in the Galaxy located within the giant molecular cl…

astro-ph.GA2021★ 7 cited

The physical and chemical structure of high-mass star-forming regions. Unraveling chemical complexity with the NOEMA large program "CORE"

C. Gieser, H. Beuther, D. Semenov +30

We use sub-arcsecond resolution (∼0.4′′) observations with NOEMA at 1.37 mm to study the dust emission and molecular gas of 18 high-mass star-forming regions. We combine the…

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