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I. Ashmore

4 papers hereh-index 454 citations9 works total

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

author position
  • first author1
  • middle author2

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph1
  • astro-ph.EP1
  • astro-ph.GA1
  • astro-ph.SR1
same name
  • I. Ashmore — 1 paper

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
20082012
most citedSputtering in oblique C-type shocks

19 citations · 49 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2012★ 19 cited

Sputtering in oblique C-type shocks

S. Van Loo, I. Ashmore, P. Caselli +2

We present the first results for the sputtering of grain mantles and cores obtained with self-consistent multifluid hydromagnetic models of C-type shocks propagating through dusty…

astro-ph.EP2009★ 10 cited

Transient evolution of C-type shocks in dusty regions of varying density

I. Ashmore, S. Van Loo, P. Caselli +2

Outflows of young stars drive shocks into dusty, molecular regions. Most models of such shocks assume that they are steady and propagating perpendicular to the magnetic field. Real…

astro-ph.SR2009★ 18 cited

Time-dependent simulations of steady C-type shocks

S. Van Loo, I. Ashmore, P. Caselli +2

Using a time-dependent multifluid, magnetohydrodynamic code, we calculated the structure of steady perpendicular and oblique C-type shocks in dusty plasmas. We included relevant pr…

astro-ph2008★ 2 cited

Dust in Interstellar Clouds, Evolved Stars and Supernovae

T. W. Hartquist, S. Van Loo, S. A. E. G. Falle +2

Outflows of pre-main-sequence stars drive shocks into molecular material within 0.01 - 1 pc of the young stars. The shock-heated gas emits infrared, millimeter and submillimeter li…

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