A phase change in X Persei

التفاصيل البيبلوغرافية
العنوان: A phase change in X Persei
المؤلفون: S. J. Unger, Victor Reglero, P. Roche, M. J. Gorrod, J. Kastner, Andrew Norton, B. J. Payne, M. J. Coe, Amando Estela, Juan Fabregat
المصدر: Monthly Notices of the Royal Astronomical Society. 253:579-583
بيانات النشر: Oxford University Press (OUP), 1991.
سنة النشر: 1991
مصطلحات موضوعية: Physics, Absorption spectroscopy, Infrared, Be star, Astrophysics::High Energy Astrophysical Phenomena, X-ray binary, Astronomy, Balmer series, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, symbols.namesake, Apparent magnitude, Space and Planetary Science, symbols, Astrophysics::Solar and Stellar Astrophysics, H-alpha, Astrophysics::Earth and Planetary Astrophysics, Emission spectrum, Astrophysics::Galaxy Astrophysics
الوصف: We present a series of optical spectroscopic and infrared photometric observations of the Be/X-ray binary system X Per made over the last four years. Over this period the Hα line profile changed from emission to absorption, accompanied by a decrease in the infrared flux by over a magnitude and a flattening of the infrared spectrum. Such behaviour is consistent with the loss of the circumstellar disc or shell of material around the Be star and the reversion to a normal O/B-type star.
تدمد: 1365-2966
0035-8711
URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_________::0a3c535fb61cd198912bab2b9b132e21
https://doi.org/10.1093/mnras/253.4.579
حقوق: OPEN
رقم الأكسشن: edsair.doi...........0a3c535fb61cd198912bab2b9b132e21
قاعدة البيانات: OpenAIRE