posted on 2016-11-18, 14:33authored byA. Somero, P. Hakala, G. A. Wynn
RS Ophiuchi (RS Oph) is a symbiotic variable and a recurrent nova (RN). We have monitored it with the Nordic Optical Telescope and obtained 30 high-resolution (R = 46 000) optical spectra over one orbital cycle during quiescence. To our knowledge, this is the best-sampled high-resolution spectroscopic data set of RS Oph over one orbital period. We do not detect any direct signatures of an accretion disc such as double peaked emission lines, but many line profiles are complex consisting of superimposed emission and absorption components. We measure the spin of the red giant and conclude that it is tidally locked to the binary orbit. We observe Na I absorption features, probably arising from the circumbinary medium, that has been shaped by previous RN outbursts. We do not detect any intrinsic polarization in the optical wavelengths.
Funding
AS acknowledges funding from the European Commission under
the Marie Curie Host Fellowships Action for Early Stage Research
Training SPARTAN programme Contract No MEST-CT-
2004-007512, University of Leicester, UK; the Finnish Graduate
School in Astronomy and Space Physics; and Academy of Finland
grant 277375. This work is based on observations made with the
Nordic Optical Telescope, operated on the island of La Palma jointly
by Denmark, Finland, Iceland, Norway, and Sweden, in the Spanish
Observatorio del Roque de los Muchachos of the Instituto de Astrofisica
de Canarias. The data presented here were obtained in part
with ALFOSC, which is provided by the Instituto de Astrofisica
de Andalucia (IAA) under a joint agreement with the University of
Copenhagen and NOTSA. We acknowledge with thanks the variable
star observations from the AAVSO International Database contributed
by observers worldwide and used in this research.
History
Citation
Monthly Notices of the Royal Astronomical Society, (January 21, 2017) 464 (3): 2784-2795.
Author affiliation
/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy
Version
VoR (Version of Record)
Published in
Monthly Notices of the Royal Astronomical Society
Publisher
Oxford University Press (OUP), Royal Astronomical Society