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M. Young

7 papers hereh-index 6505 citations12 works total

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

author position
  • sole author1
  • first author6

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

fields
  • astro-ph.SR3
  • astro-ph1
  • astro-ph.EP1
  • astro-ph.HE1
  • astro-ph.IM1
same name
  • M. Young — 47 papers, h 23
  • M. Young — 37 papers, h 9
  • M. Young — 20 papers, h 14
  • M. Young — 15 papers, h 9
  • M. Young — 12 papers, h 9
  • M. Young — 8 papers, h 13

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
20032015
most citedPulsar magnetic alignment and the pulsewidth-age relation

65 citations · 181 across the 5 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2015★ 49 cited

Binary accretion rates: dependence on temperature and mass-ratio

Matthew D. Young, Cathie J. Clarke

We perform a series of 2D smoothed particle hydrodynamics (SPH) simulations of gas accretion onto binaries via a circumbinary disc, for a range of gas temperatures and binary mass…

astro-ph.SR2015

Dependence of fragmentation in self-gravitating accretion discs on small scale structure

Matthew D. Young, Cathie J. Clarke

We propose a framework for understanding the fragmentation criterion for self-gravitating discs which, in contrast to studies that emphasise the `gravoturbulent' nature of such dis…

astro-ph.SR2014★ 33 cited

The evolution of the mass ratio of accreting binaries: the role of gas temperature

Matthew D. Young, Jonathon T. Baird, Cathie J. Clarke

We explore an unresolved controversy in the literature about the accuracy of Smoothed Particle Hydrodynamics (SPH) in modeling the accretion of gas onto a binary system, a problem…

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