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Marie-Luise Steinmeyer

3 papers here

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

author position
  • first author2
  • middle author1

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

fields
  • astro-ph.EP3
ORCID 0000-0003-0605-0263

identity via Semantic Scholar / OpenAlex

most citedSublimation of refractory minerals in the gas envelopes of accreting rocky planets

15 citations · 23 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.EP2024★ 8 cited

The GAPS programme at TNG LXIV: An inner eccentric sub-Neptune and an outer sub-Neptune-mass candidate around BD+00 444 (TOI-2443)

L. Naponiello, A. S. Bonomo, L. Mancini +25

We examined in depth the star BD+00 444 (GJ 105.5, TOI-2443; V = 9.5 mag; d = 23.9 pc), with the aim of characterizing and confirming the planetary nature of its small companion, t…

astro-ph.EP2024

Vapor equilibrium models of accreting rocky planets demonstrate direct core growth by pebble accretion

Marie-Luise Steinmeyer, Anders Johansen

The gaseous envelope of an accreting rocky planet becomes hot enough to sublimate silicates and other refractory minerals. For this work, we studied the effect of the resulting env…

astro-ph.EP2023★ 15 cited

Sublimation of refractory minerals in the gas envelopes of accreting rocky planets

Marie-Luise Steinmeyer, Peter Woitke, Anders Johansen

Protoplanets growing within the protoplanetary disk by pebble accretion acquire hydrostatic gas envelopes. Due to accretion heating, the temperature in these envelopes can become h…

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