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researcher

A. Castellanos-Ramírez

4 papers hereh-index 218 citations6 works total

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

author position
  • first author2
  • middle author1
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
  • astro-ph.SR1
same name
  • A. Castellanos-Ramírez — 3 papers
  • A. Castellanos-Ramírez — 3 papers, h 3

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
20182021
most citedTwo-wind interactions in binaries with two orbiting giant stars

7 citations · 7 across the 1 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2021★ 7 cited

Two-wind interactions in binaries with two orbiting giant stars

A. Castellanos-Ramírez, A. Rodríguez-González, Z. Meliani +3

Some red giant envelopes present spiral structures (seen either in dust scattered stellar continuum or in molecular line emission), the most striking example probably being AFGL 30…

astro-ph.SR2021

Velocity segregation in a clump-like outflow with a non-top hat velocity cross-section

A. Castellanos-Ramírez, A. C. Raga, J. Cantó +2

High velocity clumps joined to the outflow source by emission with a "Hubble law" ramp of linearly increasing radial velocity vs. distance are observed in some planetary nebulae an…

astro-ph.GA2019

Numerical models for the dust in RCW 120

A. Rodríguez-González, Z. Meliani, M. Sánchez-Cruces +2

The interstellar bubble RCW 120 seen around a type O runaway star is driven by the stellar wind and the ionising radiation emitted by the star. The boundary between the stellar win…

astro-ph.GA2018

Kinematics of the Galactic Bubble RCW 120

Mónica Sánchez-Cruces, Antonio Castellanos-Ramírez, Margarita Rosado +2

We studied the kinematics of the Galactic bubble RCW 120 in the [SII]λλ$6717,6731Ålines. We measured a LSR radial velocity ranging from ~-74 to ~-6km/s. We found evidence of expans…

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