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Christiane Helling

3 papers here

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

author position
  • middle author2
  • last author1

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

fields
  • astro-ph.EP3
same name
  • Christiane Helling — 9 papers, h 6
  • Christiane Helling — 8 papers, h 10
  • Christiane Helling — 7 papers, h 2
  • Christiane Helling — 4 papers, h 12
  • Christiane Helling — 4 papers, h 5
  • Christiane Helling — 3 papers, h 6

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
20232025
most citedA grid of self-consistent MSG (MARCS-StaticWeather-GGchem) cool stellar, sub-stellar, and exoplanetary model atmospheres

3 citations · 3 across the 1 of their papers we have counts for

collaborators

3 papers

astro-ph.EP2025

The MSG model for cloudy substellar atmospheres: A grid of self-consistent substellar atmosphere models with microphysical cloud formation

Beatriz Campos Estrada, David A. Lewis, Christiane Helling +3

State-of-the-art JWST observations are unveiling unprecedented views into the atmospheres of substellar objects in the infrared, further highlighting the importance of clouds. Curr…

astro-ph.EP2024★ 3 cited

A grid of self-consistent MSG (MARCS-StaticWeather-GGchem) cool stellar, sub-stellar, and exoplanetary model atmospheres

Uffe G. Jørgensen, Flavia Amadio, Beatriz Campos Estrada +8

Computation of a grid of self consistent 1D model atmospheres of cool stars, sub-stellar objects and exoplanets in the effective temperature range 300K to 3000K, including cloud fo…

astro-ph.EP2023

On the likely magnesium-iron silicate dusty tails of catastrophically evaporating rocky planets

Beatriz Campos Estrada, James E. Owen, Marija R. Jankovic +2

Catastrophically evaporating rocky planets provide a unique opportunity to study the composition of small planets. The surface composition of these planets can be constrained via m…

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