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E. Santamar'ia

2 papers hereh-index 310 citations7 works total

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

author position
  • first author1
  • middle author1

Across the 2 of 2 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR2
same name
  • E. Santamar'ia — 6 papers, h 6
  • E. Santamar'ia — 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

most citedSpatio-kinematic models of five nova remnants: correlations between nova shell axial ratio, expansion velocity, and speed class

9 citations · 15 across the 2 of their papers we have counts for

collaborators

2 papers

astro-ph.SR2022★ 6 cited

Planetary nebulae with Wolf-Rayet-type central stars -- IV. NGC 1501 and its mixing layer

G. Rubio, J. Toalá, H. Todt +4

Theory predicts that the temperature of the X-ray-emitting gas (∼106 K) detected from planetary nebulae (PNe) is a consequence of mixing or thermal conduction when in con…

astro-ph.SR2022★ 9 cited

Spatio-kinematic models of five nova remnants: correlations between nova shell axial ratio, expansion velocity, and speed class

E. Santamaría, M. A. Guerrero, S. Zavala +3

We present long-slit intermediate-dispersion spectroscopic observations and narrow-band direct imaging of four classical nova shells, namely TAur, HRDel, DQHer and QUVul, and the n…

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