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S. Cazaux

3 papers here

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

fields
  • astro-ph.EP2
  • astro-ph.SR1
ORCID 0000-0003-0320-3578
same name
  • S. Cazaux — 14 papers, h 22
  • S. Cazaux — 10 papers, h 18
  • S. Cazaux — 4 papers, h 9
  • S. Cazaux — 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

most citedPore evolution in interstellar ice analogues: simulating the effects of temperature increase

46 citations · 73 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.EP2022★ 13 cited

Ices in planet-forming disks: Self-consistent ice opacities in disk models

Aditya M. Arabhavi, Peter Woitke, Stephanie M. Cazaux +3

In cold and shielded environments, molecules freeze out on dust grain surfaces to form ices such as H2O, CO, CO2, CH4, CH3OH, and NH3. In protoplanetary disks, the exact radial and…

astro-ph.EP2022★ 14 cited

Circumplanetary disk ices. I. Ice formation vs. viscous evolution and grain drift

Nickolas Oberg, Inga Kamp, Stephanie Cazaux +2

The large icy moons of Jupiter formed in a circumplanetary disk (CPD). CPDs are fed by infalling circumstellar gas and dust which may be shock-heated upon accretion or sublimated w…

astro-ph.SR2014★ 46 cited

Pore evolution in interstellar ice analogues: simulating the effects of temperature increase

S. Cazaux, J. -B. Bossa, H. Linnartz +1

Context. The level of porosity of interstellar ices - largely comprised of amorphous solid water (ASW) - contains clues on the trapping capacity of other volatile species and deter…

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