Zobrazeno 1 - 10
of 49
pro vyhledávání: '"Ömür Çakırlı"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society.
Binarity and pulsations are two notable properties that frequently appear together in massive stars. To place constraints on how binarity affects stellar evolution, the exact parameters of massive stars in binary systems must be known. Their exact an
Autor:
Ömür Çakırlı, Barış Hoyman
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 509:5511-5522
The study of detached eclipsing binaries in open clusters can provide powerful tests of theoretical stellar evolutionary models. These models must simultaneously fit the masses, radii, and radiative properties of the eclipsing stars with essentially
Autor:
Ömür Çakırlı, Barış Hoyman
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 493:2329-2338
Solar-type stars in eclipsing binaries are proving to be a remarkable resource of knowledge for testing models of stellar evolution, as spectroscopic and photometric studies have opened up a window into their interiors. Until recently, many cases hav
Publikováno v:
New Astronomy. 68:10-19
We analyzed high-precision Kepler photometry and high-resolution UVES and GIRAFFE spectroscopy from ESO Science Archieve for a double-lined eclipsing binary star in the field of the high metallicity old open cluster NGC 6791. Earlier measurements of
We present results of the combined photometric and spectroscopic analysis of four systems that are eclipsing binaries with a twin component (mass ratio q similar or equal to 1). These are exceptional tools to provide information for probing the inter
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::937ec0cb421aa0f36c5d3ced8dad8b22
https://hdl.handle.net/11454/77343
https://hdl.handle.net/11454/77343
We employ optical spectroscopy and Kepler photometry to derive the physical properties and pulsational characteristics of the detached system KIC 2557430. We find that the system is formed by F-type components. Combining results from the analysis of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3d81adb9e457ed9fdc2be51d67c7cdf8
https://hdl.handle.net/11454/62769
https://hdl.handle.net/11454/62769
Red giant stars are proving to be an exceptional source of information for testing models of stellar evolution, as photometric and spectroscopic analysis has opened up a window into their interiors, providing an exciting chance to develop highly cons
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c7a857daf8a7169302bd07d33b2049d7
https://hdl.handle.net/11454/62183
https://hdl.handle.net/11454/62183
Publikováno v:
New Astronomy. 62:70-84
2-s2.0-85044657063
We present the first comprehensive catalog of the ? Doradus type pulsating stars. This catalog covers observational properties of all ? Dor variables obtained until January 2017. The photometric and physical properties of 109
We present the first comprehensive catalog of the ? Doradus type pulsating stars. This catalog covers observational properties of all ? Dor variables obtained until January 2017. The photometric and physical properties of 109
Publikováno v:
New Astronomy. 52:96-107
We present new spectroscopic observations of the double-lined eclipsing binary V850 Cyg. The long-cadence photometric observations obtained by Kepler were analysed and combined with the analysis of radial velocities for deriving the absolute paramete
Publikováno v:
New Astronomy. 46:47-53
We present spectroscopic and photometric study of V421 Peg. This eclipsing binary displays lines from both components that are well separated. This allowed us to classify the primary and secondary component as F(1 ± 0.5) V and F(2 ± 0.5) V, respect