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researcher

C. Chandler

81 papers hereh-index 436.5k citations197 works total

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

author position
  • first author4
  • middle author64
  • last author7

Across the 75 of 81 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR34
  • astro-ph22
  • astro-ph.GA16
  • astro-ph.EP7
  • astro-ph.HE1
  • astro-ph.IM1
same name
  • C. Chandler — 54 papers, h 12
  • C. Chandler — 15 papers, h 5
  • C. Chandler — 2 papers, h 3
  • C. Chandler — 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
19952023
most citedSpiral Density Waves in a Young Protoplanetary Disk

346 citations · 5.8k across the 80 of their papers we have counts for

collaborators
Showing 2012 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2012★ 182 cited

The Co-ordinated Radio and Infrared Survey for High-Mass Star Formation - II. Source Catalogue

C. R. Purcell, M. G. Hoare, W. D. Cotton +27

The CORNISH project is the highest resolution radio continuum survey of the Galactic plane to date. It is the 5 GHz radio continuum part of a series of multi-wavelength surveys tha…

astro-ph.GA2012★ 183 cited

The Co-ordinated Radio and Infrared Survey for High Mass Star Formation (The CORNISH Survey) - I. Survey Design

M. G. Hoare, C. R. Purcell, E. B. Churchwell +26

We describe the motivation, design and implementation of the CORNISH survey, an arcsecond resolution radio continuum survey of the inner Galactic plane at 5 GHz using the Karl G. J…

astro-ph.GA2012★ 93 cited

Complex Structure in Class 0 Protostellar Envelopes III: Velocity Gradients in Non-Axisymmetric Envelopes, Infall or Rotation?

John J. Tobin, Lee Hartmann, Edwin A. Bergin +5

We present an interferometric kinematic study of morphologically complex protostellar envelopes based on observations of the dense gas tracers N2H+ and NH3. The strong asymmetric n…

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