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T. Peters

46 papers hereh-index 232.7k citations115 works total

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

author position
  • sole author1
  • first author16
  • middle author24
  • last author3

Across the 44 of 46 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA30
  • astro-ph.SR12
  • astro-ph1
  • astro-ph.EP1
  • astro-ph.IM1
  • physics.flu-dyn1
same name
  • T. Peters — 19 papers, h 11
  • T. Peters — 15 papers, h 15
  • T. Peters — 9 papers, h 9
  • T. Peters — 8 papers, h 54
  • T. Peters — 3 papers, h 4
  • T. Peters — 3 papers, 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
20072022
most citedThe SILCC (SImulating the LifeCycle of molecular Clouds) project - II. Dynamical evolution of the supernova-driven ISM and the launching of outflows

233 citations · 2.3k across the 46 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★ 19 cited

Fragmentation in the massive G31.41+0.31 protocluster

M. T. Beltrán, V. M. Rivilla, R. Cesaroni +18

Context. ALMA observations at 1.4 mm and 0.2'' (750au) angular resolution of the Main core in the high-mass star forming region G31.41+0.31 have revealed a puzzling scenario: on th…

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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