Zobrazeno 1 - 10
of 14
pro vyhledávání: '"L. M. Sharipova"'
Publikováno v:
Odessa Astronomical Publications, Vol 12, Iss 0, Pp 197-200 (2017)
We present the review of different properties of several close binary systems, based on our observations. These binaries are as follow: SU UMa type stars V503 Cyg and V1504 Cyg, X-Ray novae V518 Per and V404 Cyg. They have the extremal mass ratio of
Externí odkaz:
https://doaj.org/article/4c1575d20f9c4075be8cc20233b51d0c
Publikováno v:
Odessa Astronomical Publications, Vol 9, Iss 0, Pp 117-118 (2017)
The original slitless spectrograph are created in the Crimean Astrophysical Observatory for 0.5-m meniscus telescope. It has three replaceable transparent diffraction gratings with the distance control. The highsensitive TV tube intensified isocon is
Externí odkaz:
https://doaj.org/article/a8cd0d222341428e8fe74bc1643a476b
Autor:
L. M. Sharipova
Publikováno v:
Bulletin of the Lebedev Physics Institute. 49:436-439
Autor:
L. M. Sharipova
Publikováno v:
Astrophysics. 62:439-451
The character of the interaction of two gaseous components which are a structural feature of the nucleus of the Seyfert galaxy NGC 1275 is established during the epoch of a minimum in its activity. A bank of emission line profiles (Hβ and O[III] λ5
Autor:
L. M. Sharipova
Publikováno v:
Astrophysics. 61:289-300
This is a study of the main spectral characteristics (profiles, relative intensities, and equivalent widths) of the brightest emission lines of the nucleus of the Seyfert galaxy NGC7469 in different phases of its activity. Spectral data obtained with
Publikováno v:
Astrophysics. 59:48-56
The spectral characteristics of radiation from the nucleus of the Seyfert galaxy NGC 1275 are studied on a long time scale. Changes in the profiles of some emission lines and changes in the relative intensities of hydrogen and forbidden lines and the
Autor:
A. I. Galeev, E. A. Nikolaeva, I. F. Bikmaev, V. V. Shimansky, L. M. Sharipova, S. S. Melnikov, R. Ya. Zhuchkov, E. N. Irtuganov, S. Grebenev, N. Sakhibullin
We present the results of our long-term photometric and spectroscopic observations at the Russian-Turkish RTT-150 telescope for the optical counterpart to one of the best-known sources, representatives of the class of fast X-ray transients, IGR J1754
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::723806975ce4f7682fa627ffe6d4b313
https://aperta.ulakbim.gov.tr/record/49665
https://aperta.ulakbim.gov.tr/record/49665
Publikováno v:
Astronomical & Astrophysical Transactions. 25:415-418
The results of the emission line study of the optical spectrum of the Seyfert galaxy NGC 3227 nucleus are presented. 53 spectra obtained during the maximum nucleus brightness on 12–15 January 1977 with the 6 m telescope were the basis of the invest
Publikováno v:
Astrophysics. 49:427-436
This is a study of optical emission lines of the nucleus of the Seyfert galaxy NGC 3227. This work is based on 53 spectrograms obtained with the 6-m telescope at the brightness maximum of this galactic nucleus on January 12–15, 1977. A set of profi
Autor:
L. M. Sharipova, V. V. Prokof'eva
Publikováno v:
Astronomical & Astrophysical Transactions. 17:433-437
Spectrophotometric observations of the nucleus of the galaxy NGC 4151, the reference star and spectrophotometric standards were carried out at the Crimean Astrophysical Observatory during 13 nights in 1988 (January 23 – June 10). The slitless spect