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researcher

R. Zavala

42 papers hereh-index 242.5k citations116 works total

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

author position
  • sole author1
  • first author3
  • middle author20
  • last author9

Across the 33 of 42 papers where every author was matched, so the position is known.

fields
  • astro-ph18
  • astro-ph.SR18
  • astro-ph.CO3
  • astro-ph.GA2
  • astro-ph.IM1
same name
  • R. Zavala — 2 papers, h 6

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
20012021
most citedA Compact Supermassive Binary Black Hole System

439 citations · 2.6k across the 42 of their papers we have counts for

collaborators
Showing 2013Show all

3 papers · 1 filter

astro-ph.GA2013★ 8 cited

A Multi-wavelength Study of the Host Environment of SMBHB 4C+37.11

Roger W. Romani, W. R. Forman, Christine Jones +4

4C+37.11, at z=0.055 shows two compact radio nuclei, imaged by VLBI at 7mas separation, making it the closest known resolved super-massive black hole binary (SMBHB). An important q…

astro-ph.SR2013★ 29 cited

An interferometric study of the post-AGB binary 89 Herculis I Spatially resolving the continuum circumstellar environment at optical and near-IR wavelengths with the VLTI, NPOI, IOTA, PTI, and the CHARA Array

M. Hillen, T. Verhoelst, H. Van Winckel +9

Binary post-AGB stars are interesting laboratories to study both the evolution of binaries as well as the structure of circumstellar disks. A multiwavelength high angular resolutio…

astro-ph.SR2013★ 35 cited

Dynamical mass of the O-type supergiant in Zeta Orionis A

C. A. Hummel, Th. Rivinius, M. -F. Nieva +3

A close companion of Zeta Orionis A was found in 2000 with the Navy Precision Optical Interferometer (NPOI), and shown to be a physical companion. Because the primary is a supergia…

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