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Rebecca G. Martin

101 papers hereh-index 261.9k citations111 works total

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

author position
  • sole author2
  • first author46
  • middle author27
  • last author23

Across the 98 of 101 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP65
  • astro-ph.SR15
  • astro-ph.HE13
  • astro-ph7
  • astro-ph.GA1
same name
  • Rebecca G. Martin — 24 papers, h 4
  • Rebecca G. Martin — 9 papers
  • Rebecca G. Martin — 6 papers, h 3
  • Rebecca G. Martin — 4 papers, h 2

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
20062026
most citedOn the Evolution of the Snow Line in Protoplanetary Discs

154 citations · 3.2k across the 99 of their papers we have counts for

collaborators
Showing 2013Show all

4 papers · 1 filter

astro-ph.EP2013★ 65 cited

Two timescale dispersal of magnetized protoplanetary disks

Philip J. Armitage, Jacob B. Simon, Rebecca G. Martin

Protoplanetary disks are likely to be threaded by a weak net flux of vertical magnetic field that is a remnant of the much larger fluxes present in molecular cloud cores. If this f…

astro-ph.SR2013★ 24 cited

The gravo-magneto disc instability with a viscous dead zone

Rebecca G. Martin, Stephen H. Lubow

We consider the evolution of accretion discs that contain some turbulence within a disc dead zone, a region about the disc midplane of a disc that is not sufficiently ionised for t…

astro-ph.EP2013★ 52 cited

Formation of circumbinary planets in a dead zone

Rebecca G. Martin, Philip J. Armitage, Richard D. Alexander

Circumbinary planets have been observed at orbital radii where binary perturbations may have significant effects on the gas disk structure, on planetesimal velocity dispersion, and…

astro-ph.SR2013★ 44 cited

Propagation of the Gravo-Magneto Disc Instability

Rebecca G. Martin, Stephen H. Lubow

Discs that contain dead zones are subject to the Gravo-Magneto (GM) instability that arises when the turbulence shifts from gravitational to magnetic. We have previously described…

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