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researcher

V. Guzmán

29 papers hereh-index 201k citations35 works total

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

author position
  • first author2
  • middle author23

Across the 25 of 29 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP20
  • astro-ph.GA5
  • astro-ph.SR4
same name
  • V. Guzmán — 26 papers, h 19
  • V. Guzmán — 8 papers, h 3
  • V. Guzmán — 6 papers, h 3
  • V. Guzmán — 6 papers, h 5
  • V. Guzmán — 3 papers, h 4

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
20152026
most citedMolecules with ALMA at Planet-forming Scales (MAPS) V: CO gas distributions

176 citations · 1.1k across the 28 of their papers we have counts for

collaborators
Showing 2023Show all

3 papers · 1 filter

astro-ph.SR2023★ 30 cited

The Perseus ALMA Chemical Survey (PEACHES). III. Sulfur-bearing species tracing accretion and ejection processes in young protostars

E. Artur de la Villarmois, V. V. Guzman, Y. -L. Yang +2

(Abridged) Sulfur chemistry is poorly understood in the process of low-mass star and planet formation, where the main carriers of sulfur are still unknown. Despite the fact that si…

astro-ph.EP2023★ 18 cited

Molecules with ALMA at Planet-forming Scales (MAPS). Complex Kinematics in the AS 209 Disk Induced by a Forming Planet and Disk Winds

Maria Galloway-Sprietsma, Jaehan Bae, Richard Teague +19

We study the kinematics of the AS 209 disk using the J=2-1 transitions of 12CO, 13CO, and C18O. We derive the radial, azimuthal, and vertical velocity of the gas, ta…

astro-ph.EP2023★ 17 cited

A gap-sharing planet pair shaping the crescent in HD 163296: a disk sculpted by a resonant chain

Juan Garrido-Deutelmoser, Cristobal Petrovich, Carolina Charalambous +2

ALMA observations of the disk around HD 163296 have resolved a crescent-shape substructure at around 55 au, inside and off-center from a gap in the dust that extends from 38 au to…

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