Context. Despite their large number in the Galaxy, M dwarfs remain elusive objects and the modeling of their photosphere has long remained a challenge (molecular opacities, dust cloud formation). Aims. Our objectives are to validate the BT-Settl model at
Abstract About 70% of stars in the Milky Way galaxy are M-dwarfs. They span a range of low masses (...
International audienceContext. Being the most numerous and oldest stars in the galaxy, M dwarfs are ...
Abstract About 70% of stars in the Milky Way galaxy are M-dwarfs. They span a range of low masses (...
Context. Despite their large number in the Galaxy, M dwarfs remain elusive objects and the modeling ...
International audienceWe present an optical spectral atlas of stars covering the whole M-dwarf seque...
International audienceWe present a comparison of low-resolution spectra of 60 stars covering the who...
International audienceContext. M dwarfs are an important source of information when studying and pro...
Abstract About 70% of stars in the Milky Way galaxy are M-dwarfs. They span a range of low masses (...
International audienceContext. Being the most numerous and oldest stars in the galaxy, M dwarfs are ...
Abstract About 70% of stars in the Milky Way galaxy are M-dwarfs. They span a range of low masses (...
Context. Despite their large number in the Galaxy, M dwarfs remain elusive objects and the modeling ...
International audienceWe present an optical spectral atlas of stars covering the whole M-dwarf seque...
International audienceWe present a comparison of low-resolution spectra of 60 stars covering the who...
International audienceContext. M dwarfs are an important source of information when studying and pro...
Abstract About 70% of stars in the Milky Way galaxy are M-dwarfs. They span a range of low masses (...
International audienceContext. Being the most numerous and oldest stars in the galaxy, M dwarfs are ...
Abstract About 70% of stars in the Milky Way galaxy are M-dwarfs. They span a range of low masses (...