Reference : Coordinated monitoring of the eccentric O-star binary Iota Orionis: optical spectroscopy...
Scientific journals : Article
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/15942
Coordinated monitoring of the eccentric O-star binary Iota Orionis: optical spectroscopy and photometry
English
Marchenko, Sergey V [Département de Physique and Observatoire du Mont Mégantic, Université de Montréal, CP 6128, Succursale Centre-Ville, Montréal, QC H3C 3J7, Canada]
Rauw, Grégor mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Groupe d'astrophysique des hautes énergies (GAPHE) - Sciences spatiales >]
Antokhina, Eleonora A [Moscow State University, Sternberg State Astronomical Institute, Universitetskij Prospect 13, 119899, Moscow, Russia]
Antokhin, Igor I [Moscow State University, Sternberg State Astronomical Institute, Universitetskij Prospect 13, 119899, Moscow, Russia]
Ballereau, Dominique [Observatoire de Paris-Meudon, DASGAL/UMR 8633, F-92125 Meudon Principal Cedex, France]
Chauville, Jacques [Observatoire de Paris-Meudon, DASGAL/UMR 8633, F-92125 Meudon Principal Cedex, France]
Corcoran, Michael F [Universities Space Research Association/Laboratory for High Energy Astrophysics, GSFC, Greenbelt, MD 20771, USA]
Costero, Rafael [Instituto de Astronomía, Universidad Nacional Autónoma de México, J. J. Tablada 1006, Colonia Lomas de Santa Maria, 58090 Morelia, Michoacán, Mexico]
Echevarria, Juan [Instituto de Astronomía, Universidad Nacional Autónoma de México, J. J. Tablada 1006, Colonia Lomas de Santa Maria, 58090 Morelia, Michoacán, Mexico]
Eversberg, Thomas [Département de Physique and Observatoire du Mont Mégantic, Université de Montréal, CP 6128, Succursale Centre-Ville, Montréal, QC H3C 3J7, Canada]
Gayley, Ken G [University of Iowa, 203 van Allen Hall, Iowa City, IA 52245, USA]
Koenigsberger, Gloria [Instituto de Astronomía, Universidad Nacional Autónoma de México, J. J. Tablada 1006, Colonia Lomas de Santa Maria, 58090 Morelia, Michoacán, Mexico]
Miroshnichenko, Anatoly S [Ritter Observatory, The University of Toledo, Toledo, OH 43606, USA]
Moffat, Anthony F J [Département de Physique and Observatoire du Mont Mégantic, Université de Montréal, CP 6128, Succursale Centre-Ville, Montréal, QC H3C 3J7, Canada]
Morrell, Nidia I [Observatorio de La Plata, 1900 La Plata, Argentina]
Morrison, Nancy D [Ritter Observatory, The University of Toledo, Toledo, OH 43606]
Mulliss, Christopher L [Ritter Observatory, The University of Toledo, Toledo, OH 43606]
Pittard, Julian M [School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT]
Stevens, Ian R [School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT]
Vreux, Jean-Marie mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > > ]
Zorec, Jean [Institut d'Astrophysique, 98bis boulevard Arago, 75014 Paris, France]
1-Sep-2000
Monthly Notices of the Royal Astronomical Society
Blackwell Publishing
317
333-342
International
0035-8711
Oxford
United Kingdom
[en] BINARIES: GENERAL ; STARS: EARLY-TYPE ; STARS: GENERAL ; STARS: INDIVIDUAL: IOTA ORIONIS
[en] With the objective of investigating the wind-wind collision phenomenon and supporting contemporaneous X-ray observations, we have organized a large-scale, coordinated optical monitoring campaign of the massive, highly eccentric O9III+B1III binary Iota Orionis. Successfully separating the spectra of the components, we refine the orbital elements and confirm the rapid apsidal motion in the system. We also see strong interaction between the components during periastron passage and detect phase-locked variability in the spectrum of the secondary star. However, we find no unambiguous signs of the bow shock crashing on the surface of the secondary, despite the predictions of hydrodynamic simulations. Combining all available photometric data, we find rapid, phase-locked variations and model them numerically, thus restricting the orbital inclination to 50°<~i<~70°.
http://hdl.handle.net/2268/15942
10.1046/j.1365-8711.2000.03542.x
http://adsabs.harvard.edu/abs/2000MNRAS.317..333M

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