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E. Montiel

31 papers hereh-index 182.2k citations55 works total

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

author position
  • first author2
  • middle author23
  • last author2

Across the 27 of 31 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR13
  • astro-ph.GA7
  • astro-ph.CO6
  • astro-ph.EP2
  • astro-ph.HE2
  • astro-ph.IM1
same name
  • E. Montiel — 16 papers, h 12
  • E. Montiel — 5 papers
  • E. Montiel — 4 papers, h 2
  • E. Montiel — 3 papers, h 2
  • E. Montiel — 3 papers, h 4
  • E. Montiel — 2 papers, 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
20092023
most citedHerschel Detects a Massive Dust Reservoir in Supernova 1987A

368 citations · 2k across the 30 of their papers we have counts for

collaborators
Showing 2014 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2014★ 132 cited

Dust and Gas in the Magellanic Clouds from the HERITAGE Herschel Key Project. II. Gas-to-Dust Ratio Variations across ISM Phases

Julia Roman-Duval, Karl Gordon, Margaret Meixner +32

The spatial variations of the gas-to-dust ratio (GDR) provide constraints on the chemical evolution and lifecycle of dust in galaxies. We examine the relation between dust and gas…

astro-ph.GA2014★ 70 cited

The influence of supernova remnants on the interstellar medium in the Large Magellanic Cloud seen at 20--600 μm wavelengths

Maša Lakićević, Jacco Th. van Loon, Margaret Meixner +20

We present the analysis of supernova remnants (SNRs) in the Large Magellanic Cloud (LMC) and their influence on the environment at far-infrared (FIR) and submillimeter wavelengths.…

astro-ph.GA2014★ 176 cited

Dust and Gas in the Magellanic Clouds from the HERITAGE Herschel Key Project. I. Dust Properties and Insights into the Origin of the Submm Excess Emission

Karl D. Gordon, Julia Roman-Duval, Caroline Bot +33

The dust properties in the Large and Small Magellanic Clouds are studied using the HERITAGE Herschel Key Project photometric data in five bands from 100 to 500 micron. Three simple…

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