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E. Mamonova

4 papers hereh-index 242 citations8 works total

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

fields
  • astro-ph.EP2
  • astro-ph.SR2
same name
  • E. Mamonova — 4 papers, h 1

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 citedForming rocky exoplanets around K-dwarf stars

5 citations · 13 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2025★ 1 cited

Young M dwarfs flare activity model: Towards better exoplanetary atmospheric characterisation

E. Mamonova, A. F. Kowalski, K. Herbst +2

Context. Stellar flares can significantly influence the atmospheres and habitability of orbiting exoplanets, especially around young and active M dwarfs. Understanding the temporal…

astro-ph.EP2025★ 4 cited

Planets similar in size are often dissimilar in interior

E. Mamonova, Y. Shan, P. Hatalova +1

Recent works have found evidence of significant intrasystem uniformity in planet properties such as radius, mass, and orbital spacing, collectively termed 'peas in a pod' trends. I…

astro-ph.SR2025★ 3 cited

Flare frequency in M dwarfs belonging to Young Moving Groups

E. Mamonova, Y. Shan, A. F. Kowalski +1

Context. M stars are preferred targets for studying terrestrial exoplanets, for which we hope to obtain their atmosphere spectra in the next decade. However, M dwarfs have long bee…

astro-ph.EP2023★ 5 cited

Forming rocky exoplanets around K-dwarf stars

P. Hatalova, R. Brasser, E. Mamonova +1

How multiple close-in super-Earths form around stars with masses lower than that of the Sun is still an open issue. Several recent modeling studies have focused on planet formation…

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