activity
20032026
most citedA distance to the Large Magellanic Cloud that is precise to one per cent

686 citations · 4.7k across the 116 of their papers we have counts for

collaborators
Showing 2018Show all

9 papers · 1 filter

astro-ph.IM2018★ 4 cited

Perspectives of a visible instrument on the VLTI

Florentin Millour, Denis Mourard, Julien Woillez +9

In this paper we present the most promising science cases for a new generation visible instrument on the VLTI and the conceptual idea for the instrumental configuration. We also pr…

astro-ph.SR2018★ 67 cited

The effect of metallicity on Cepheid Period-Luminosity relations from a Baade-Wesselink analysis of Cepheids in the Milky Way and Magellanic Clouds

W. Gieren, J. Storm, P. Konorski +14

The extragalactic distance scale builds on the Cepheid period-luminosity (PL) relation. In this paper, we want to carry out a strictly differential comparison of the absolute PL re…

astro-ph.SR2018★ 5 cited

CRIRES high-resolution infrared spectroscopy of the long-period Cepheid l Car

N. Nardetto, E. Poretti, A. Gallenne +17

The dynamical structure of the atmosphere of Cepheids has been well studied in the optical. Several authors have found very interesting spectral features in the J band, but little…

astro-ph.SR2018

Optical interferometry and Gaia parallaxes for a robust calibration of the Cepheid distance scale

Pierre Kervella, Antoine Mérand, Alexandre Gallenne +5

We present the modeling tool we developed to incorporate multi-technique observations of Cepheids in a single pulsation model: the Spectro-Photo-Interferometry of Pulsating Stars (…

astro-ph.SR2018★ 49 cited

The Araucaria Project: High-precision Cepheid astrophysics from the analysis of variables in double-lined eclipsing binaries

Bogumił Pilecki, Wolfgang Gieren, Grzegorz Pietrzyński +15

Based on new observations and improved modeling techniques, we have reanalyzed seven Cepheids in the Large Magellanic Cloud. Improved physical parameters have been determined for t…

astro-ph.SR2018★ 20 cited

Physical properties of beta Lyr A and its opaque accretion disk

D. Mourard, M. Broz, J. Nemravova +23

Mass exchange and mass loss in close binaries can significantly affect their evolution, but a complete self-consistent theory of these processes is still to be developed. Processes…