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E. De Beck

53 papers hereh-index 8204 citations27 works total

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

author position
  • first author8
  • middle author37
  • last author5

Across the 50 of 53 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR46
  • astro-ph.GA4
  • astro-ph.IM3
same name
  • E. De Beck — 10 papers

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
20102026
most citedProbing the mass-loss history of AGB and red supergiant stars from CO rotational line profiles - II. CO line survey of evolved stars: derivation of mass-loss rate formulae

242 citations · 1.8k across the 49 of their papers we have counts for

collaborators
Showing 2021Show all

3 papers · 1 filter

astro-ph.SR2021★ 38 cited

ATOMIUM: ALMA tracing the origins of molecules in dust forming oxygen rich M-type stars: Motivation, sample, calibration, and initial results

C. A. Gottlieb, L. Decin, A. M. S. Richards +33

This overview paper presents ATOMIUM, a Large Programme in Cycle 6 with the Atacama Large Millimeter-submillimeter Array (ALMA). The goal of ATOMIUM is to understand the dynamics a…

astro-ph.SR2021★ 9 cited

Multiple components in the molecular outflow of the red supergiant NML Cyg

Holly Andrews, Elvire De Beck, Per Hirvonen

Despite their large impact on stellar and galactic evolution, the properties of outflows from red supergiants are not well characterised. We used the Onsala 20m telescope to perfor…

astro-ph.SR2021★ 21 cited

ATOMIUM: Halide molecules around the S-type AGB star W Aquilae

T. Danilovich, M. Van de Sande, J. M. C. Plane +36

S-type asymptotic giant branch (AGB) stars are thought to be intermediates in the evolution of oxygen- to carbon-rich AGB stars. The chemical compositions of their circumstellar en…

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