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M dwarfs are key targets for high-resolution spectroscopic analyses due to a high incidence of these stars in the solar neighbourhood and their importance as exoplanetary hosts. Several methodological challenges make such analyses difficult, leading
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::12cf539567d138fb2726fb072743d915
The symbiotic star R Aqr is part of a small sample of binary AGB stars observed with ALMA. The sample stars are: R Aqr, Mira, W Aql, and pi1 Gru. The sample covers a range in binary separation and wind properties, where R Aqr is the source with the s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2d3bd9785c4b5fa253af0cd77edc1195
http://arxiv.org/abs/1806.04979
http://arxiv.org/abs/1806.04979