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researcher

A. Maeder

143 papers hereh-index 5413.1k citations396 works total

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

author position
  • sole author11
  • first author28
  • middle author50
  • last author45

Across the 134 of 143 papers where every author was matched, so the position is known.

fields
  • astro-ph68
  • astro-ph.SR52
  • gr-qc9
  • astro-ph.CO5
  • astro-ph.GA4
  • astro-ph.EP3
same name
  • A. Maeder — 11 papers, h 3
  • A. Maeder — 10 papers, h 4
  • A. Maeder — 5 papers
  • A. Maeder — 4 papers, h 3
  • A. Maeder — 3 papers, h 6
  • A. Maeder — 1 paper, h 21

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
19952023
most citedGrids of stellar models with rotation - I. Models from 0.8 to 120 Msun at solar metallicity (Z = 0.014)

1.7k citations · 10.1k across the 139 of their papers we have counts for

collaborators
Showing 2000Show all

4 papers · 1 filter

astro-ph2000★ 4 cited

Stellar evolution with rotation VI: The Eddington and Omega-limits, the rotational mass loss for OB and LBV stars

Andre Maeder, Georges Meynet

Several properties of massive stars with large effects of rotation and radiation are studied. We show that there are 2 roots for the equation giving the rotational velocities at br…

astro-ph2000★ 59 cited

Stellar Evolution with Rotation V: Changes in all the Outputs of Massive Star Models

Georges Meynet, Andre Maeder

Grids of models for rotating stars are constructed in the range of 9 to 120 M⊙​ at solar metallicity. The following effects of rotation are included: shellular rotation, ne…

astro-ph2000

On the Formation of Massive Stars by Accretion

Peder Norberg, Andre Maeder

(Abriged) At present, there are two scenarios for the formation of massive stars: 1) The accretion scenario and 2) The coalescence scenario, which implies the merging of intermedia…

astro-ph2000★ 844 cited

The evolution of rotating stars

Andre Maeder, Georges Meynet

First, we review the main physical effects to be considered in the building of evolutionary models of rotating stars on the Upper Main-Sequence (MS). The internal rotation law evol…

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