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researcher

A. Ahmadi

39 papers hereh-index 16768 citations64 works total

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

author position
  • first author3
  • middle author24
  • last author2

Across the 29 of 39 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA25
  • astro-ph.SR14
same name
  • A. Ahmadi — 6 papers, h 6
  • A. Ahmadi — 6 papers, h 5
  • A. Ahmadi — 5 papers, h 4
  • A. Ahmadi — 3 papers, h 27
  • A. Ahmadi — 2 papers, h 8
  • A. Ahmadi — 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
20162026
most citedSubstructures in the Keplerian disc around the O-type (proto)star G17.64+0.16

79 citations · 503 across the 26 of their papers we have counts for

collaborators
Showing 2023Show all

3 papers · 1 filter

astro-ph.GA2023

Density distributions, magnetic field structures and fragmentation in high-mass star formation

H. Beuther, C. Gieser, J. D. Soler +19

Methods: Observing the large pc-scale Stokes I mm dust continuum emission with the IRAM 30m telescope and the intermediate-scale (<0.1pc) polarized submm dust emission with the Sub…

astro-ph.GA2023★ 25 cited

Kinematics and stability of high-mass protostellar disk candidates at sub-arcsecond resolution -- Insights from the IRAM NOEMA large program CORE

Aida Ahmadi, H. Beuther, F. Bosco +28

The fragmentation mode of high-mass molecular clumps and the accretion processes that form the most massive stars (M≳8M⊙​) are still not well understood. To this end,…

astro-ph.GA2023★ 20 cited

Physical and chemical complexity in high-mass star-forming regions with ALMA. I. Overview and evolutionary trends of physical properties

Caroline Gieser, Henrik Beuther, Dmitry Semenov +3

In this study, we investigate how physical properties, such as the density and temperature profiles, evolve on core scales through the evolutionary sequence during high-mass star f…

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