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Mónica Rodríguez

12 papers hereh-index 8257 citations12 works total

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

author position
  • sole author1
  • first author4
  • middle author3
  • last author4

Across the 12 of 12 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA7
  • astro-ph2
  • astro-ph.SR2
  • astro-ph.CO1
same name
  • Mónica Rodríguez — 4 papers, h 1
  • Mónica Rodríguez — 1 paper, h 1
  • Mónica Rodríguez — 1 paper, 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
20042020
most citedOxygen enrichment in carbon-rich planetary nebulae

71 citations · 326 across the 12 of their papers we have counts for

collaborators
Showing 2011Show all

4 papers · 1 filter

astro-ph.GA2011★ 1 cited

C/O Abundance Ratios and Dust Features in Galactic Planetary Nebulae

G. Delgado-Inglada, M. Rodríguez

The iron depletion factors found in Galactic planetary nebulae (PNe) span over two orders of magnitude, suggesting that there are differences in the grain formation and destruction…

astro-ph.GA2011★ 1 cited

Chlorine and Sulfur in Nearby Planetary Nebulae and H II Regions

Mónica Rodríguez, Gloria Delgado-Inglada

We derive the chlorine abundances in a sample of nearby planetary nebulae (PNe) and H II regions that have some of the best available spectra. We use a nearly homogeneous procedure…

astro-ph.GA2011★ 17 cited

The Oxygen Abundance in the Solar Neighborhood

Mónica Rodríguez, Gloria Delgado-Inglada

We present a homogeneous analysis of the oxygen abundance in five H II regions and eight planetary nebulae (PNe) located at distances lower than 2 kpc and with available spectra of…

astro-ph.GA2011

An overabundance of oxygen in planetary nebulae of the solar neighborhood

Mónica Rodríguez, Gloria Delgado-Inglada

We study the oxygen abundance in five H II regions and seven planetary nebulae (PNe) located within 2 kpc from the Sun that have available spectra of high quality. Our analysis use…

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