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SF2A-2013: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics

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The article was published on 2013-11-01 and is currently open access. It has received 230 citations till now.

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Influence of Rotation on Stellar Evolution

TL;DR: In this article, a review of the different physical processes associated to rotation that are expected to impact the evolution of stars is presented. And the authors describe in detail the way these physical processes are introduced in 1D stellar evolution codes and how their introduction in the modelling has impacted our understanding of the internal structure, nucleosynthesis and global evolution of the stars.
Journal ArticleDOI

General relativistic observables for the ACES experiment

TL;DR: In this paper, the relativistic coordinate transformations that are needed to describe the motion of the Atomic Clock Ensemble in Space (ACES) in Earth orbit and to compute observable quantities were developed.
Journal ArticleDOI

TOI-150b and TOI-163b: two transiting hot Jupiters, one eccentric and one inflated, revealed by TESS near and at the edge of the JWST CVZ

Diana Kossakowski, +58 more
TL;DR: In this paper, the authors presented the discovery of two hot Jupiters, namely TOI-150b and HD271181b, using 30-min cadence Transiting Exoplanet Survey Satellite (TESS) photometry from Sector 1 and thoroughly characterized through follow-up photometry (CHAT, Hazelwood, LCO/CTIO, El Sauce, TRAPPIST-S), high-resolution spectroscopy (FEROS, CORALIE), confirming the planetary nature of two signals.
Journal ArticleDOI

A General Relativistic External Compton-Scattering Model for TeV Emission from M87

TL;DR: In this article, a self-consistent EIC model was proposed to explain the flat TeV spectrum of M87 within the framework of fully general relativity, where the background soft photons were from the advection-dominated accretion flo w (ADAF) around the central black hole, and the high energy electrons are from the mini-jets which are powered by the magnetic reconnection in the main jet.
Journal ArticleDOI

Mode classification in fast-rotating stars using a convolutional neural network: model-based regular patterns in δ Scuti stars

TL;DR: In this article, a convolutional neural network was used to sort the thousands of oscillation modes obtained from the spectra of fast-rotating Scuti stars and retrieve the observational scaling law.
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