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V2368 Ophiuchi : an eclipsing and double-lined spectroscopic binary used as a photometric comparison star for U Ophiuchi


Harmanec, P.; Božić, Hrvoje; Mayer, P.; Eenens, P; Brož, M.; Wolf, M.; Yang, S.; Šlechta, M.; Ruždjak, Domagoj; Sudar, Davor; Ak, H.
V2368 Ophiuchi : an eclipsing and double-lined spectroscopic binary used as a photometric comparison star for U Ophiuchi // Astronomy and astrophysics, 531 (2011), A49-1 doi:10.1051/0004-6361/201116610 (međunarodna recenzija, članak, znanstveni)


Naslov
V2368 Ophiuchi : an eclipsing and double-lined spectroscopic binary used as a photometric comparison star for U Ophiuchi

Autori
Harmanec, P. ; Božić, Hrvoje ; Mayer, P. ; Eenens, P ; Brož, M. ; Wolf, M. ; Yang, S. ; Šlechta, M. ; Ruždjak, Domagoj ; Sudar, Davor ; Ak, H.

Izvornik
Astronomy and astrophysics (0004-6361) 531 (2011); A49-1

Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni

Ključne riječi
Stars: early-type; binaries: close; stars: individual: V2368 Oph; stars: individual: U Oph; binaries: spectroscopic

Sažetak
The A-type star HR 6412 = V2368 Oph was used by several investigators as a photometric comparison star for the known eclipsing binary U Oph but was found to be variable by three independent groups, including us. By analysing series of new spectral and photometric observations and a critical compilation of available radial velocities, we were able to find the correct period of light and radial-velocity variations and demonstrate that the object is an eclipsing and double-lined spectroscopic binary moving in a highly eccentric orbit. We derived a linear ephemeris Tmin.I = HJD (2 454 294.67 ± 0.01) + (3832712 ± 000004) ×   E and estimated preliminary basic physical properties of the binary. The dereddened UBV magnitudes and effective temperatures of the primary and secondary, based on our light- and velocity-curve solutions, led to distance estimates that agree with the Hipparcos distance within the errors. We find that the mass ratio must be close to one, but the limited number and wavelength range of our current spectra does not allow a truly precise determination of the binary masses. Nevertheless, our results show convincingly that both binary components are evolved away from the main sequence, which makes this system astrophysically very important. There are only a few similarly evolved A-type stars among known eclipsing binaries. Future systematic observations and careful analyses can provide very stringent tests for the stellar evolutionary theory.

Izvorni jezik
Engleski

Znanstvena područja
Fizika



POVEZANOST RADA


Projekt / tema
007-0000000-1362 - Eruptivni procesi u Sunčevoj atmosferi (Bojan Vršnak, )
007-0000000-1364 - Fizikalni procesi u atmosferama Sunca i zvijezda (Vladimir Ruždjak, )

Ustanove
Geodetski fakultet, Zagreb

Časopis indeksira:


  • Current Contents Connect (CCC)
  • Web of Science Core Collection (WoSCC)
    • SCI-EXP, SSCI i/ili A&HCI
  • Scopus


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