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L. Maud

36 papers hereh-index 191k citations63 works total

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

author position
  • first author3
  • middle author25
  • last author1

Across the 29 of 36 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA22
  • astro-ph.SR13
  • astro-ph.EP1
same name
  • L. Maud — 15 papers, h 11
  • L. Maud — 14 papers, h 10
  • L. Maud — 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
20122025
most citedDisk evolution in the solar neighborhood. I Disk frequencies from 1 to 100 Myr

183 citations · 1.5k across the 36 of their papers we have counts for

collaborators
Showing 2023Show all

3 papers · 1 filter

astro-ph.GA2023★ 9 cited

FAUST X: Formaldehyde in the Protobinary System [BHB2007] 11: Small Scale Deuteration

Lucy Evans, Charlotte Vastel, Francisco Fontani +16

Context. Deuterium in H-bearing species is enhanced during the early stages of star formation, however, only a small number of high spatial resolution deuteration studies exist tow…

astro-ph.GA2023★ 22 cited

ALMA-IMF. VII. First release of the full spectral line cubes: Core kinematics traced by DCN J=(3-2)

N. Cunningham, A. Ginsburg, R. Galván-Madrid +30

ALMA-IMF is an Atacama Large Millimeter/submillimeter Array (ALMA) Large Program designed to measure the core mass function (CMF) of 15 protoclusters chosen to span their early evo…

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,…

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