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researcher

M. Beltrán

9 papers hereh-index 460 citations11 works total

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

author position
  • middle author8

Across the 8 of 9 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA6
  • astro-ph.SR2
  • astro-ph.IM1
same name
  • M. Beltrán — 56 papers, h 34
  • M. Beltrán — 20 papers, h 6
  • M. Beltrán — 10 papers, h 7
  • M. Beltrán — 6 papers, h 3
  • M. Beltrán — 6 papers, h 3
  • M. Beltrán — 4 papers, h 3

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
20102026
most citedYoung starless cores embedded in the magnetically dominated Pipe Nebula

49 citations · 79 across the 9 of their papers we have counts for

collaborators
Showing 2026Show all

3 papers · 1 filter

astro-ph.SR2026

Magnetic fields in Massive Star-Forming Regions (MagMaR). VIII. Magnetic field overrun by gravity in GGD 27's accretion streamers

M. Fernández-López, J. A. López-Vázquez, J. M. Girart +20

Context. Accretion streamers connected to protostellar disks and/or envelopes are thought to transport material across several thousand of au. Whether the motions of the gas compri…

astro-ph.GA2026

The dominance of turbulence over magnetism in the formation of massive star cluster seeds

Junhao Liu, Patricio Sanhueza, Piyali Saha +32

High-mass stars form in protoclusters, where gravo-magnetic processes shape collapsing clouds and clumps to be elongated preferentially perpendicular to magnetic (B) fields. Yet it…

astro-ph.SR2026★ 5 cited

Digging into the Interior of Hot Cores with ALMA (DIHCA). VII. Disk candidates around high-mass stars and evidence of anisotropic infall

Fernando A. Olguin, Patricio Sanhueza, Yoko Oya +19

We study the kinematics of condensations in 30 fields forming high-mass stars with ALMA at a high-resolution of ~0.08'' on average (~230 au). The presence of disks is important for…

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