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Radial velocity measurements of the runaway stars AE Aur and ι Ori
Author(s) -
Heyne Therese,
Mugrauer M.,
Bischoff R.,
Wagner D.,
Neuhäuser R.,
Hoffmann S. M.,
Lux O.
Publication year - 2020
Publication title -
astronomische nachrichten
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.394
H-Index - 63
eISSN - 1521-3994
pISSN - 0004-6337
DOI - 10.1002/asna.202013808
Subject(s) - physics , radial velocity , astrophysics , stars , spectrograph , astronomy , observatory , galaxy , proper motion , binary number , spectral line , arithmetic , mathematics
We present the results of our spectroscopic monitoring observations of the late O‐type runaway stars AE Aur and ι Ori, carried out between September 2016 and May 2018 using the Échelle spectrograph FLECHAS at the University Observatory Jena. For both stars, we obtained current radial velocity (RV) measurements with better precision than before. These results can be used for further advanced calculations of their space motion, needed to determine, for example, their place of origin in our Galaxy. In this paper, we describe the observations and the data reduction, as well as the analysis of all spectral data. We find a stable RV for AE Aur and confirm ι Ori as a double‐lined spectroscopic binary and derive its current Keplerian orbital elements.