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researcher

E. Vázquez-Semadeni

74 papers hereh-index 395k citations140 works total

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

author position
  • sole author12
  • first author14
  • middle author26
  • last author14

Across the 66 of 74 papers where every author was matched, so the position is known.

fields
  • astro-ph40
  • astro-ph.GA31
  • astro-ph.CO1
  • astro-ph.SR1
  • physics.flu-dyn1
same name
  • E. Vázquez-Semadeni — 33 papers, h 15
  • E. Vázquez-Semadeni — 5 papers, h 3
  • E. Vázquez-Semadeni — 1 paper, h 2

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
19962026
most citedDensity probability distribution in one-dimensional polytropic gas dynamics

364 citations · 5.3k across the 73 of their papers we have counts for

collaborators
Showing 2012Show all

4 papers · 1 filter

astro-ph.GA2012★ 8 cited

Applying a one-dimensional PDR model to the Taurus molecular cloud and its atomic envelope

J. S. Heiner, E. Vázquez-Semadeni

In this contribution, we test our previously published one-dimensional PDR model for deriving total hydrogen volume densities from HI column density measurements in extragalactic r…

astro-ph.GA2012★ 23 cited

Interstellar MHD Turbulence and Star Formation

Enrique Vazquez-Semadeni

This chapter reviews the nature of turbulence in the Galactic interstellar medium (ISM) and its connections to the star formation (SF) process. The ISM is turbulent, magnetized, se…

astro-ph.GA2012★ 19 cited

From dusty filaments to massive stars: The case of NGC 7538 S

Raul Naranjo-Romero, Luis A. Zapata, Enrique Vazquez-Semadeni +3

We report on high-sensitivity and high-angular resolution archival Submillimeter Array (SMA) observations of the large (∼15000 AU) putative circumstellar disk associated with…

astro-ph.GA2012

Physical Processes of Interstellar Turbulence

Enrique Vazquez-Semadeni

I discuss the role of self-gravity and radiative heating and cooling in shaping the nature of the turbulence in the interstellar medium (ISM) of our galaxy. The heating and cooling…

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