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M. Rosenthal

7 papers hereh-index 7119 citations8 works total

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

author position
  • first author5
  • middle author1
  • last author1

Across the 7 of 7 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP7
same name
  • M. Rosenthal — 11 papers, h 8
  • M. Rosenthal — 8 papers, h 9
  • M. Rosenthal — 2 papers, h 4
  • M. Rosenthal — 2 papers, h 3
  • M. Rosenthal — 2 papers, h 6
  • M. Rosenthal — 2 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
20182020
most citedNew Constraints From Dust Lines On The Surface Densities Of Protoplanetary Disks

62 citations · 149 across the 7 of their papers we have counts for

collaborators
Showing 2018Show all

2 papers · 1 filter

astro-ph.EP2018★ 15 cited

Restrictions on the Growth of Gas Giant Cores via Pebble Accretion

M. M. Rosenthal, R. A. Murray-Clay

We apply an order-of-magnitude model of gas-assisted growth, known as pebble accretion, in a turbulent medium to suggest a reason why some systems form wide orbital separation gas…

astro-ph.EP2018★ 14 cited

Gas-Assisted Growth of Protoplanets in a Turbulent Medium

M. M. Rosenthal, R. A. Murray-Clay, H. B. Perets +1

Pebble accretion is a promising process for decreasing growth timescales of planetary cores, allowing gas giants to form at wide orbital separations. However, nebular turbulence ca…

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