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researcher

A. Esquivel

4 papers here

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

author position
  • middle author1
  • last author2

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph2
  • astro-ph.GA1
  • astro-ph.HE1
ORCID 0000-0001-7222-1492
same name
  • A. Esquivel — 32 papers, h 20
  • A. Esquivel — 18 papers, h 8
  • A. Esquivel — 4 papers, h 2
  • A. Esquivel — 4 papers, h 6
  • A. Esquivel — 2 papers, h 1
  • A. Esquivel — 2 papers, h 0

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
20012022
most citedA latitude-dependent wind model for Mira's cometary head

19 citations · 48 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2022★ 17 cited

Rectangular core-collapse supernova remnants: application to Puppis A

D. M. -A. Meyer, P. F. Velazquez, O. Petruk +9

Core-collapse supernova remnants are the gaseous nebulae of galactic interstellar media (ISM) formed after the explosive death of massive stars. Their morphology and emission prope…

astro-ph.GA2016★ 8 cited

The time evolution of HH 1 from four epochs of HST images

A. C. Raga, B. Reipurth, A. Esquivel +1

We present an analysis of four epochs of Hα and [S II] λλ 6716/6731 HST images of HH 1. For determining proper motions we explore a new method based on analysis of spatially de…

astro-ph2008★ 19 cited

A latitude-dependent wind model for Mira's cometary head

A. C. Raga, J. Cantó, F. De Colle +4

We present a 3D numerical simulation of the recently discovered cometary structure produced as Mira travels through the galactic ISM. In our simulation, we consider that Mira eject…

astro-ph2001★ 4 cited

Quest for HI Turbulence Statistics: New Techniques

A. Lazarian, D. Pogosyan, Alejandro Esquivel

HI data cubes are sources of unique information on interstellar turbulence. Doppler shifts due to supersonic motions contain information on turbulent velocity field which is otherw…

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