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T. Möller

9 papers hereh-index 13619 citations32 works total

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

author position
  • first author1
  • middle author4
  • last author3

Across the 8 of 9 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA6
  • astro-ph.SR2
  • astro-ph.IM1
same name
  • T. Möller — 12 papers, h 45
  • T. Möller — 10 papers, h 6
  • T. Möller — 9 papers, h 0
  • T. Möller — 5 papers
  • T. Möller — 2 papers, h 7
  • T. Möller — 2 papers, h 3

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
20122024
most citedThe Physical and chemical structure of Sagittarius B2 -- IV. Converging filaments in the high-mass cluster forming region Sgr B2(N)

53 citations · 342 across the 9 of their papers we have counts for

collaborators
Showing 2019Show all

3 papers · 1 filter

astro-ph.SR2019★ 53 cited

Chemical complexity in high-mass star formation: An observational and modeling case study of the AFGL 2591 VLA 3 hot core

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

We present a detailed observational and modeling study of the hot core VLA 3 in the high-mass star-forming region AFGL 2591, which is a target region of the NOrthern Extended Milli…

astro-ph.GA2019★ 38 cited

The physical and chemical structure of Sagittarius B2 -- V. Non-thermal emission in the envelope of Sgr B2

F. Meng, Á. Sánchez-Monge, P. Schilke +8

The giant molecular cloud Sagittarius B2 (hereafter SgrB2) is the most massive region with ongoing high-mass star formation in the Galaxy. In the southern region of the 40-pc large…

astro-ph.GA2019★ 53 cited

The Physical and chemical structure of Sagittarius B2 -- IV. Converging filaments in the high-mass cluster forming region Sgr B2(N)

A. Schwörer, Á. Sánchez-Monge, P. Schilke +7

We have used an unbiased, spectral line-survey that covers the frequency range from 211 to 275 GHz and was obtained with ALMA (angular resolution of 0.4 arcsec) to study the small-…

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