Kretschmar, PeterPeterKretschmarMartínez-Núñez, SilviaSilviaMartínez-NúñezBozzo, EnricoEnricoBozzoOskinova, Lidia M.Lidia M.OskinovaPuls, JoachimJoachimPulsSIDOLI, LaraLaraSIDOLISundqvist, Jon OlofJon OlofSundqvistBlay, PerePereBlayFalanga, MaurizioMaurizioFalangaFürst, FelixFelixFürstGímenez-García, AngelAngelGímenez-GarcíaKreykenbohm, IngoIngoKreykenbohmKühnel, MatthiasMatthiasKühnelSander, AndreasAndreasSanderTorrejón, José MiguelJosé MiguelTorrejónWilms, JörnJörnWilmsPodsiadlowski, PhilippPhilippPodsiadlowskiManousakis, AntoniosAntoniosManousakis2020-09-012020-09-012017978-1-107-17006-31743-9213http://hdl.handle.net/20.500.12386/27021Strong winds from massive stars are a topic of interest to a wide range of astrophysical fields. In High-Mass X-ray Binaries the presence of an accreting compact object on the one side allows to infer wind parameters from studies of the varying properties of the emitted X-rays; but on the other side the accretor's gravity and ionizing radiation can strongly influence the wind flow. Based on a collaborative effort of astronomers both from the stellar wind and the X-ray community, this presentation attempts to review our current state of knowledge and indicate avenues for future progress.STAMPAenConference paper10.1017/S17439213170024112-s2.0-85046974324000455603400057https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/stellar-winds-in-massive-xray-binaries/44EDCB0D1B24049CD236389F61ED3C612017IAUS..329..355KFIS/05 - ASTRONOMIA E ASTROFISICA