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researcher

M. Persson

16 papers hereh-index 241.9k citations55 works total

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

author position
  • first author2
  • middle author7
  • last author2

Across the 11 of 16 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR10
  • astro-ph.GA6
same name
  • M. Persson — 10 papers, h 52
  • M. Persson — 5 papers, h 4
  • M. Persson — 4 papers, h 8
  • M. Persson — 3 papers, h 31
  • M. Persson — 2 papers, h 3
  • M. Persson — 2 papers, h 12

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
20122021
most citedThe VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars. A Statistical Characterization of Class 0 and I Protostellar Disks

332 citations · 741 across the 7 of their papers we have counts for

collaborators
Showing 2020Show all

3 papers · 1 filter

astro-ph.SR2020

Missing water in Class I protostellar disks

Daniel Harsono, Magnus Persson, Alyssa Ramos +10

Water is a key volatile that provides insights into the initial stages of planet formation. The low water abundances inferred from water observations toward low-mass protostellar o…

astro-ph.GA2020

Seeds of Life in Space (SOLIS). VI. Chemical evolution of sulfuretted species along the outflows driven by the low-mass protostellar binary NGC1333-IRAS4A

Vianney Taquet, Claudio Codella, Marta de Simone +8

Context. Low-mass protostars drive powerful molecular outflows that can be observed with mm and sub-mm telescopes. Various sulfuretted species are known to be bright in shocks and…

astro-ph.GA2020★ 332 cited

The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars. A Statistical Characterization of Class 0 and I Protostellar Disks

John J. Tobin, Patrick Sheehan, S. Thomas Megeath +33

We have conducted a survey of 328 protostars in the Orion molecular clouds with ALMA at 0.87 mm at a resolution of ∼0.1" (40 au), including observations with the VLA at 9 mm t…

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