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Physical Parameters of the Detached Eclipsing Binary KIC3858884 with a delta-Scuti Type Pulsating Component


Lee, Chung-Uk; Kim, S.-L.; Lee, J.W.; Pavlovski, Krešimir; Southworth, John
Physical Parameters of the Detached Eclipsing Binary KIC3858884 with a delta-Scuti Type Pulsating Component // From Interacting Binaries to Exoplanets: Essential Modeling Tools, Proceedings IAU Symposium 282 / Richards, Mercedes T. ; Hubeny, Ivan (ur.).
Cambridge: Cambridge University Press, 2012. str. 327-328 (poster, međunarodna recenzija, cjeloviti rad (in extenso), znanstveni)


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Naslov
Physical Parameters of the Detached Eclipsing Binary KIC3858884 with a delta-Scuti Type Pulsating Component

Autori
Lee, Chung-Uk ; Kim, S.-L. ; Lee, J.W. ; Pavlovski, Krešimir ; Southworth, John

Vrsta, podvrsta i kategorija rada
Radovi u zbornicima skupova, cjeloviti rad (in extenso), znanstveni

Izvornik
From Interacting Binaries to Exoplanets: Essential Modeling Tools, Proceedings IAU Symposium 282 / Richards, Mercedes T. ; Hubeny, Ivan - Cambridge : Cambridge University Press, 2012, 327-328

Skup
International Astronomical Union Symposium 282

Mjesto i datum
Vysoké Tatry, Slovačka, 18.07.2011. - 22.07.2011

Vrsta sudjelovanja
Poster

Vrsta recenzije
Međunarodna recenzija

Ključne riječi
stars; fundamental parameters; oscillations; eclipsing binaries

Sažetak
We present physical parameters for the detached eclipsing binary KIC3858884 which has a δ-Scuti type pulsating secondary component. To derive orbital elements from the radial-velocity curve, high resolution Echelle spectra were obtained at the Bohyunsan Optical Astronomy Observatory in Korea. The BOES spectra and Kepler photometric data were analyzed with well-known codes: JKTEBOP and Wilson-Devinney model for eclipsing light-curve synthesis, and Period04 for pulsation frequency analysis. After the iterative curve fitting, we determined the physical parameters of KIC3858884 as M1=2.02 ± 0.23M, M2=2.02 ± 0.16M, R1=3.61 ± 0.12R, R2=2.84 ± 0.10R, respectively.

Izvorni jezik
Engleski

Znanstvena područja
Fizika



POVEZANOST RADA


Projekti:
119-0000000-3135 - Struktura i evolucija zvijezda (Pavlovski, Krešimir, MZOS ) ( CroRIS)

Ustanove:
Prirodoslovno-matematički fakultet, Zagreb

Profili:

Avatar Url Krešimir Pavlovski (autor)


Citiraj ovu publikaciju:

Lee, Chung-Uk; Kim, S.-L.; Lee, J.W.; Pavlovski, Krešimir; Southworth, John
Physical Parameters of the Detached Eclipsing Binary KIC3858884 with a delta-Scuti Type Pulsating Component // From Interacting Binaries to Exoplanets: Essential Modeling Tools, Proceedings IAU Symposium 282 / Richards, Mercedes T. ; Hubeny, Ivan (ur.).
Cambridge: Cambridge University Press, 2012. str. 327-328 (poster, međunarodna recenzija, cjeloviti rad (in extenso), znanstveni)
Lee, C., Kim, S., Lee, J., Pavlovski, K. & Southworth, J. (2012) Physical Parameters of the Detached Eclipsing Binary KIC3858884 with a delta-Scuti Type Pulsating Component. U: Richards, M. & Hubeny, I. (ur.)From Interacting Binaries to Exoplanets: Essential Modeling Tools, Proceedings IAU Symposium 282.
@article{article, author = {Lee, Chung-Uk and Kim, S.-L. and Lee, J.W. and Pavlovski, Kre\v{s}imir and Southworth, John}, year = {2012}, pages = {327-328}, keywords = {stars, fundamental parameters, oscillations, eclipsing binaries}, title = {Physical Parameters of the Detached Eclipsing Binary KIC3858884 with a delta-Scuti Type Pulsating Component}, keyword = {stars, fundamental parameters, oscillations, eclipsing binaries}, publisher = {Cambridge University Press}, publisherplace = {Vysok\'{e} Tatry, Slova\v{c}ka} }
@article{article, author = {Lee, Chung-Uk and Kim, S.-L. and Lee, J.W. and Pavlovski, Kre\v{s}imir and Southworth, John}, year = {2012}, pages = {327-328}, keywords = {stars, fundamental parameters, oscillations, eclipsing binaries}, title = {Physical Parameters of the Detached Eclipsing Binary KIC3858884 with a delta-Scuti Type Pulsating Component}, keyword = {stars, fundamental parameters, oscillations, eclipsing binaries}, publisher = {Cambridge University Press}, publisherplace = {Vysok\'{e} Tatry, Slova\v{c}ka} }




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