Zobrazeno 1 - 10
of 37
pro vyhledávání: '"Esin Soydugan"'
In this study, investigation of two double-lined binary stars KIC 5113146 and KIC 5111815 in NGC 6819 is presented based on both photometric and spectroscopic data. Simultaneous analysis of light and radial velocity curves was made and the absolute p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::818f955c6700edc2763d6475f99c86e8
Investigation Of Near-Contact Semi-Detached Binary Wumi Through Observations And Evolutionary Models
W UMi is a near contact, semi-detached, double-lined eclipsing binary star with an orbital period of 1.7 days. Simultaneous analysis of new BVR multi-color light curves and radial velocity data yields the main astrophysical parameters of the binary a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b48d1bf98739a277a4ce6e3da40debcd
https://aperta.ulakbim.gov.tr/record/5169
https://aperta.ulakbim.gov.tr/record/5169
Publikováno v:
New Astronomy. 46:40-46
New CCD photometric observations of the neglected classical Algol-type binary XZ Aql were obtained over 53 nights during the observing season of 2011. Photometric elements were determined from analysis of multi-colour light curves. This first compreh
Autor:
K. R. Pollard, P. M. Kilmartin, Z. Kołaczkowski, Esin Soydugan, K. Uytterhoeven, J. H. Telting, E. Niemczura, Jakub Ostrowski, Ennio Poretti, Monica Rainer, F. Kahraman Aliçavuş, P. De Cat, L. Mantegazza, Juan Carlos Suárez
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 458:2307-2322
We present a spectroscopic survey of known and candidate $\gamma$\,Doradus stars. The high-resolution, high signal-to-noise spectra of 52 objects were collected by five different spectrographs. The spectral classification, atmospheric parameters (\te
Autor:
I. Steer, Hicran Bakiş, Faruk Soydugan, Gürkan Aslan, F. Alicavus, Esin Soydugan, Zeki Eker, Volkan Bakiş, M. Alpsoy, Selçuk Bilir
Absolute parameters of 509 main-sequence stars selected from the components of detached-eclipsing spectroscopic binaries in the Solar neighbourhood are used to study mass-luminosity, mass-radius and mass-effective temperature relations (MLR, MRR and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::639cc8bb019966930e6d3e9dd46c9e90
http://arxiv.org/abs/1807.02568
http://arxiv.org/abs/1807.02568
Autor:
Gürkan Aslan, Ian Steer, Faruk Soydugan, Mehmet Alpsoy, F. Alicavus, Esin Soydugan, Volkan Bakiş, Selçuk Bilir, Hicran Bakiş, Zeki Eker
Conventional mass-luminosity (M – L) relations are defined using 509 nearby main-sequence (MS) stars within the Solar neighborhood. A smooth mass-radius (M – R) relation was fixed from radii of MS stars appeared in literature having masses within
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::665536cae28b44d603c318fc63c0e134
https://aperta.ulakbim.gov.tr/record/32963
https://aperta.ulakbim.gov.tr/record/32963
Publikováno v:
AIP Conference Proceedings.
Asteroseismology offers an opportunity for examination and detailed understanding of the internal structure of stars by probing their pulsating modes. To obtain reliable results by asteroseismology, accurate atmospheric parameters and metallicities o
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 432:3278-3287
This paper presents results from analysing spectroscopic and multicolour photometric observations of the neglected semi-detached eclipsing binary system IO Ursae Majoris (IO UMa). For the first time, the orbital parameters of the system and fundament
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 422:1250-1262
CCD observations of 68 eclipsing binary systems, candidates for containing {\delta} Scuti components, were obtained. Their light curves are analysed using the PERIOD04 software for possible pulsational behaviour. For the systems QY Aql, CZ Aqr, TY Ca
Autor:
Esin Soydugan, S.S. Doğru, Candan Çiçek, O. Demircan, F. Alicavus, Faruk Soydugan, Ahmet Erdem
Publikováno v:
New Astronomy. 16:498-502
This paper presents new CCD Bessell BVRI light curves and photometric analysis of the Algol-type binary star TX Her. The CCD observations were carried out at Canakkale Onsekiz Mart University Observatory in 2010. New BVRI light curves from this study