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researcher

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 2016Show all

4 papers · 1 filter

astro-ph.EP2016★ 22 cited

Fragmentation of Kozai-Lidov Disks

Wen Fu, Stephen H. Lubow, Rebecca G. Martin

We analyze the gravitational instability (GI) of a locally isothermal inclined disk around one component of a binary system. Such a disk can undergo global Kozai-Lidov (KL) cycles…

astro-ph.EP2016★ 33 cited

Why are pulsar planets rare?

Rebecca G. Martin, Mario Livio, Divya Palaniswamy

Pulsar timing observations have revealed planets around only a few pulsars. We suggest that the rarity of these planets is due mainly to two effects. First, we show that the most l…

astro-ph.EP2016★ 13 cited

On the Formation of Super-Earths with Implications for the Solar System

Rebecca G. Martin, Mario Livio

We first consider how the level of turbulence in a protoplanetary disk affects the formation locations for the observed close-in super-Earths in exosolar systems. We find that a pr…

astro-ph.EP2016★ 80 cited

Planet-disc evolution and the formation of Kozai-Lidov planets

Rebecca G. Martin, Stephen H. Lubow, Chris Nixon +1

With hydrodynamical simulations we determine the conditions under which an initially coplanar planet-disc system that orbits a member of a misaligned binary star evolves to form a…

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