◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

T. Lemoult

3 papers here

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

author position
  • middle author3

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

fields
  • astro-ph.SR3

identity via Semantic Scholar / OpenAlex

most citedDynamical structure of the pulsating atmosphere of RR Lyr - I. A typical pulsation cycle

18 citations · 36 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2019★ 9 cited

Evolution of the disk of pi Aqr: from near-disappearance to a strong maximum

Y. Naze, G. Rauw, J . Guarro Flo +30

Some Be stars display important variability of the strength of the emission lines formed in their disk. This is notably the case of pi Aqr. We present here the recent evolution of…

astro-ph.SR2019★ 18 cited

Dynamical structure of the pulsating atmosphere of RR Lyr - I. A typical pulsation cycle

D. Gillet, B. Mauclaire, T. Lemoult +5

RRab stars are large amplitude pulsating stars in which the pulsation is associated with strong shock wake propagating in the atmosphere. The objective of this study is to provide…

astro-ph.SR2017★ 9 cited

First observation of Hα redshifted emission in RR Lyr

D. Gillet, B. Mauclaire, T. Garrel +10

The so-called Hα third emission occurs around pulsation phase φ=0.30. It has been observed for the first time in 2011 in some RR Lyrae stars. The emission intensity is very wea…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.