After presenting global properties of M dwarfs, the principal diagnostic of activity phenomena occurring in their atmosphere from the geometrical, energetic, and temporal points of view is stressed. Observations of sunspots, plages, flares, and activity cycles are presented. The major sources of activity are discussed with particular emphasis on the generation, intensification, and measurements of stellar magnetic fields
The Space mission DWARFS is designed to determine atmospheric composition and physical properties of...
We present high-resolution echelle spectroscopy of 676 nearby M dwarfs. Our measurements include rad...
The vast majority of stars in the nearby stellar neighborhood are M dwarfs. Their low masses and lum...
Theoretical work on the atmospheres of M dwarfs has progressed along lines parallel to those followe...
We present the results from a spectroscopic study of 1080 nearby active M dwarfs, selected by correl...
We study the relationship between Galactic location ($R, Z$) and photometric activity for 3.6 millio...
I present the results of a program to spectrophotometrically monitor the L1.5 dwarf 2MASSW J1145572+...
This PhD thesis presents work on the atmospheres of both brown dwarfs and exoplanets from an observe...
M dwarfs are the most numerous type of stars in the Universe. Their low masses and their large plane...
International audienceContext. M dwarfs are an important source of information when studying and pro...
I gave an invited talk at Extreme Solar Systems IV in REYKJAVIK, ICELAND. However, please note that ...
A study of the atmospheric parameters of a sample of M dwarfs of different kinematic populations cl...
International audienceContext. Being the most numerous and oldest stars in the galaxy, M dwarfs are ...
Despite the prevalence of M dwarfs, the smallest and most common type of main sequence star, their s...
Within less than two decades, the study of low-mass stars and brown dwarfs has bloomed int...
The Space mission DWARFS is designed to determine atmospheric composition and physical properties of...
We present high-resolution echelle spectroscopy of 676 nearby M dwarfs. Our measurements include rad...
The vast majority of stars in the nearby stellar neighborhood are M dwarfs. Their low masses and lum...
Theoretical work on the atmospheres of M dwarfs has progressed along lines parallel to those followe...
We present the results from a spectroscopic study of 1080 nearby active M dwarfs, selected by correl...
We study the relationship between Galactic location ($R, Z$) and photometric activity for 3.6 millio...
I present the results of a program to spectrophotometrically monitor the L1.5 dwarf 2MASSW J1145572+...
This PhD thesis presents work on the atmospheres of both brown dwarfs and exoplanets from an observe...
M dwarfs are the most numerous type of stars in the Universe. Their low masses and their large plane...
International audienceContext. M dwarfs are an important source of information when studying and pro...
I gave an invited talk at Extreme Solar Systems IV in REYKJAVIK, ICELAND. However, please note that ...
A study of the atmospheric parameters of a sample of M dwarfs of different kinematic populations cl...
International audienceContext. Being the most numerous and oldest stars in the galaxy, M dwarfs are ...
Despite the prevalence of M dwarfs, the smallest and most common type of main sequence star, their s...
Within less than two decades, the study of low-mass stars and brown dwarfs has bloomed int...
The Space mission DWARFS is designed to determine atmospheric composition and physical properties of...
We present high-resolution echelle spectroscopy of 676 nearby M dwarfs. Our measurements include rad...
The vast majority of stars in the nearby stellar neighborhood are M dwarfs. Their low masses and lum...