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M. Meyer

5 papers hereh-index 191.1k citations56 works total

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

author position
  • middle author1
  • last author1

Across the 2 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP4
  • astro-ph1
same name
  • M. Meyer — 47 papers, h 61
  • M. Meyer — 25 papers
  • M. Meyer — 18 papers, h 41
  • M. Meyer — 18 papers, h 50
  • M. Meyer — 14 papers
  • M. Meyer — 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
20052017
most citedOn the gap-opening criterion of migrating planets in protoplanetary disks

89 citations · 198 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.EP2017★ 45 cited

The HIP 79977 debris disk in polarized light

N. Engler, H. M. Schmid, Ch. Thalmann +40

We present observations of the known edge-on debris disk around HIP 79977 (HD 146897, F star in Upper Sco, 123 pc), taken with the ZIMPOL differential polarimeter of the SPHERE ins…

astro-ph.EP2017★ 19 cited

Orbiting a binary: SPHERE characterisation of the HD 284149 system

Mariangela Bonavita, V. D'Orazi, D. Mesa +52

In this paper we present the results of the SPHERE observation of the HD 284149 system, aimed at a more detailed characterisation of both the primary and its brown dwarf companion.…

astro-ph.EP2015★ 89 cited

On the gap-opening criterion of migrating planets in protoplanetary disks

Matej Malik, Farzana Meru, Lucio Mayer +1

We perform two-dimensional hydrodynamical simulations to quantitatively explore the torque balance criterion for gap-opening (as formulated by Crida et al. 2006) in a variety of di…

astro-ph2005

Formation and Evolution of Planetary Systems: Upper Limits the Gas Mass in HD105

D. Hollenbach, U. Gorti, M. Meyer +13

We report infrared spectroscopic observations of HD 105, a nearby (∼40 pc) and relatively young (∼30 Myr) G0 star with excess infrared continuum emission, which has bee…

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