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researcher

M. Bergemann

4 papers here

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

author position
  • sole author1

Across the 1 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
  • astro-ph.GA1
ORCID 0000-0002-9908-5571
same name
  • M. Bergemann — 4 papers, h 51
  • M. Bergemann — 1 paper, 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
20102015
most citedThe Gaia-ESO Survey: the most metal-poor stars in the Galactic bulge

73 citations · 191 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2015★ 49 cited

Gaia-ESO Survey: The analysis of pre-main sequence stellar spectra

A. C. Lanzafame, A. Frasca, F. Damiani +70

This paper describes the analysis of UVES and GIRAFFE spectra acquired by the Gaia-ESO Public Spectroscopic Survey in the fields of young clusters whose population includes pre-mai…

astro-ph.GA2014★ 67 cited

The Gaia-ESO Survey: Kinematics of seven Galactic globular clusters

C. Lardo, E. Pancino, M. Bellazzini +24

The Gaia-ESO survey is a large public spectroscopic survey aimed at investigating the origin and formation history of our Galaxy by collecting spectroscopy of representative sample…

astro-ph.SR2014★ 73 cited

The Gaia-ESO Survey: the most metal-poor stars in the Galactic bulge

L. Howes, M. Asplund, A. R. Casey +39

We present the first results of the EMBLA survey (Extremely Metal-poor BuLge stars with AAOmega), aimed at finding metal-poor stars in the Milky Way bulge, where the oldest stars s…

astro-ph.SR2010★ 2 cited

NLTE abundances of Cr in the Sun and metal-poor stars

Maria Bergemann

We investigate statistical equilibrium of Cr in the atmospheres of late-type stars. The main goal is to ascertain the reason for a systematic abundance discrepancy between Cr I and…

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