Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Ilfa A. Gabitova"'
Autor:
Ilfa A. Gabitova, Anatoly S. Miroshnichenko, Sergey V. Zharikov, Ainash Amantayeva, Serik A. Khokhlov
Publikováno v:
Galaxies, Vol 12, Iss 3, p 23 (2024)
κ Draconis is a binary system with a classical Be star as the primary component. Its emission-line spectrum consists of hydrogen lines, notably the Hα line with peak intensity ratio (V/R) variations phase-locked with the orbital period P = 61.55 da
Externí odkaz:
https://doaj.org/article/21041d2b9f0a45129e3357b01cd8d589
Autor:
Anatoly S. Miroshnichenko, Raghav Chari, Stephen Danford, Peter Prendergast, Alicia N. Aarnio, Ivan L. Andronov, Lidiia L. Chinarova, Aidan Lytle, Ainash Amantayeva, Ilfa A. Gabitova, Nadezhda L. Vaidman, Sayat S. Baktybayev, Serik A. Khokhlov
Publikováno v:
Galaxies, Vol 11, Iss 4, p 83 (2023)
There is growing evidence that many Be stars are parts of binary systems. As the B-type primaries are very fast rotators and their spectral lines may be distorted by the circumstellar material, it is not easy to measure their radial velocity directly
Externí odkaz:
https://doaj.org/article/0939e0c53bc9493280fb00a80a5eb955
Autor:
Khokhlov, Anatoly S. Miroshnichenko, Raghav Chari, Stephen Danford, Peter Prendergast, Alicia N. Aarnio, Ivan L. Andronov, Lidiia L. Chinarova, Aidan Lytle, Ainash Amantayeva, Ilfa A. Gabitova, Nadezhda L. Vaidman, Sayat S. Baktybayev, Serik A.
Publikováno v:
Galaxies; Volume 11; Issue 4; Pages: 83
There is growing evidence that many Be stars are parts of binary systems. As the B-type primaries are very fast rotators and their spectral lines may be distorted by the circumstellar material, it is not easy to measure their radial velocity directly
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=multidiscipl::c445f64b430a9e94e7aaa3476cca1f63