Abstract
We present first results of the photometric and spectroscopic investigation of the B1/B2 Herbig star HD52721 performed in 2009–2010 at three observatories: Mountain Astronomical Station (Kislovodsk)—photometry, CrAO (Crimea, Ukraine)—spectroscopy, Observatory San Pedro Martyr (Ensenada, Mexico)—high-resolution echelle-spectroscopy. We have also used photometric data from the ASAS survey for 2003–2009. Our analysis has shown that a) the object is a close binary system with the orbital period of 1.610 days composed of two components of similar spectral type (B1–B2); b) the system is surrounded by the common disk-like envelope containing azimuthal inhomogeneity rotating with the orbital period of the system. We present preliminary estimates of the system parameters and discuss its possible nature.
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Original Russian Text © M.A. Pogodin, N.G. Beskrovnaya, G.G. Valyavin, I.S. Guseva, S.E. Pavlovskiy, N. Rusomarov, O.V. Ezhkova, 2013, published in Izvestiya Krymskoi Astrofizicheskoi Observatorii, 2013, Vol. 109, pp. 38–43.
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Pogodin, M.A., Beskrovnaya, N.G., Valyavin, G.G. et al. Photometric and spectroscopic investigation of the B2E Herbig star HD52721: First results. Bull.Crim. Astrophys. Observ. 109, 23–26 (2013). https://doi.org/10.3103/S019027171301018X
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DOI: https://doi.org/10.3103/S019027171301018X